Staff Dataset Information

  X-Ray - GOES X-Ray flux 0.1-0.8 nm


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux between 0.1 and 0.8 nm as measured by the primary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.70 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead.
See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  X-Ray - GOES X-Ray flux 0.1-0.8 nm (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux between 0.05 and 0.4 nm as measured by the secondary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.85 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead.
See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  X-Ray - GOES X-Ray flux 0.05-0.4 nm


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux between 0.05 and 0.4 nm as measured by the primary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.85 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead.
See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  X-Ray - GOES X-Ray flux 0.05-0.4 nm (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux between 0.1 and 0.8 nm as measured by the secondary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.70 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead.
See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  X-Ray - GOES X-Ray Background Flux


Institution:NOAA NOAA
Division: SWPC
Predictions provider: E-SWDS
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux background between 0.1 and 0.8 nm as measured by the primary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.70 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead. See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  X-Ray - GOES X-Ray Background Flux (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: E-SWDS
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: W/m^2
Import latency: 5 + ~5 minutes.
Information: This timeline provides the X-ray flux background between 0.1 and 0.8 nm as measured by the secondary NOAA GOES satellite. Note that SWPC traditionally employs a scaling factor for this timeline: the timeline data values as published by SWPC and STAFF are in fact the measured values * 0.70 (expressed in W/m^2). For scientific purposes, the unscaled measured values should be used instead. See http://ngdc.noaa.gov/stp/satellite/goes/doc/GOES_XRS_readme.pdf (32 KB) for more information.

  EUV - Lyra Lyman Alpha


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Sun-Synchronous
Units: W/m^2
Import latency: 60 + ~60 minutes.
Information: LYRA is a solar X and UV filter photometer onboard the Proba2 satellite, designed and manufactured by a Belgian–Swiss consortium. It monitors the solar irradiance in four passbands relevant to solar physics, space weather, and aeronomy. This timeline provides very high cadence (up to 10 ms) measured values in the 120-123 nm Lyman-alpha channel. This particular channel suffers from extreme degradation.

  EUV - Lyra Aluminium


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Sun-Synchronous
Units: W/m^2
Import latency: 60 + ~60 minutes.
Information: LYRA is a solar X and UV filter photometer onboard the Proba2 satellite, designed and manufactured by a Belgian–Swiss consortium. It monitors the solar irradiance in four passbands relevant to solar physics, space weather, and aeronomy. This timeline provides very high cadence (up to 10 ms) measured values in the 190-222 nm Herzberg continuum channel. This particular channel suffers from extreme degradation.

  EUV - Lyra Herzberg


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Sun-Synchronous
Units: W/m^2
Import latency: 60 + ~60 minutes.
Information: LYRA is a solar X and UV filter photometer onboard the Proba2 satellite, designed and manufactured by a Belgian–Swiss consortium. It monitors the solar irradiance in four passbands relevant to solar physics, space weather, and aeronomy. This timeline provides very high cadence (up to 10 ms) measured values in the Aluminium channel (17-80 nm + a contribution below 5 nm, including the strong He II at 30.4 nm).

  EUV - Lyra Zirconium


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Sun-Synchronous
Units: W/m^2
Import latency: 60 + ~60 minutes.
Information: LYRA is a solar X and UV filter photometer onboard the Proba2 satellite, designed and manufactured by a Belgian–Swiss consortium. It monitors the solar irradiance in four passbands relevant to solar physics, space weather, and aeronomy. This timeline provides very high cadence (up to 10 ms) measured values in the Zirconium channel (6-20 nm + a contribution below 2 nm, rejecting He II).

  Sunspot - ISN Daily - v2 (Center)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

  Sunspot - ISN Daily - v2 (North)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Daily Northern hemisphere sunspot numbers derived by the formula: R= Ns + 10 * Ng, with Ns the number of spots and Ng the number of groups counted over the Northern hemisphere (based on the sunspot group heliographic latitude). The Northern hemisphere number is always normalized to the total number, which is the global scaling reference. The production of the Northern hemisphere numbers started only in 1992.

The conventional 0.6 Zürich scale factor is not used anymore and A. Wolfer (Wolfs successor) is now defining the scale of the entire series. This puts the Sunspot Number at the scale of raw modern counts, instead of reducing it to the level of early counts by R. Wolf.

  Sunspot - ISN Daily - v2 (South)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Daily Southern hemisphere sunspot numbers derived by the formula: R= Ns + 10 * Ng, with Ns the number of spots and Ng the number of groups counted over the Southern hemisphere (based on the sunspot group heliographic latitude). The Southern hemisphere number is always normalized to the total number, which is the global scaling reference. The production of the Sourthern hemisphere numbers started only in 1992.

The conventional 0.6 Zürich scale factor is not used anymore and A. Wolfer (Wolfs successor) is now defining the scale of the entire series. This puts the Sunspot Number at the scale of raw modern counts, instead of reducing it to the level of early counts by R. Wolf.

  Sunspot - ISN Daily - v2 (Total)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
  
Estimated ISN Daily (Total)  
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Daily total sunspot number derived by the formula: R= Ns + 10 * Ng, with Ns the number of spots and Ng the number of groups counted over the entire solar disk. No daily data are provided before 1818 because daily observations become too sparse in earlier years. Therefore, R. Wolf only compiled monthly means and yearly means for all years before 1818.

The conventional 0.6 Zürich scale factor is not used anymore and A. Wolfer (Wolfs successor) is now defining the scale of the entire series. This puts the Sunspot Number at the scale of raw modern counts, instead of reducing it to the level of early counts by R. Wolf.

EISN = prediction1 of ISN Daily (Total) The estimated international sunspot number (EISN) is a daily value obtained by a simple average over available sunspot counts from prompt stations in the SILSO network.The raw values from each station are scaled using their mean annual k personal coefficient over the last elapsed year. Therefore, compared to the monthly international sunspot number (produced on the first day of each month), the accuracy of the EISN is lower because the calculation rests on a smaller number of stations and the k scaling coefficient is only an approximation of the true k coefficient of the month.The EISN is computed every few minutes and thus evolves continuously as new observations from our worldwide network are entered into our database. The EISN thus gives a dynamical preview of the final sunspot number but is an ephemeral product. It should not be archived for long-term use. At the end of each month, those values are dropped and replaced by the provisional sunspot numbers from the full calculation for the corresponding month.

  Sunspot - ISN Monthly - v2 (North)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Monthly mean Northern hemisphere sunspot numbers obtained by taking a simple arithmetic mean of the daily Northern hemisphere sunspot numbers over all days of each calendar month. Each sunspot group is counted in the Northern hemisphere based on its heliographic latitude. NB: Northern hemisphere numbers are always normalized to the corresponding total monthly mean sunspot number.

  Sunspot - ISN Monthly Smoothed - v2 (South)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Monthly smoothed mean Southern hemisphere sunspot numbers. The 13-month smoothed monthly sunspot numbers are derived by a tapered-boxcar running mean of monthly Southern hemisphere sunspot numbers over 13 months centered on the corresponding month (Smoothing function: equal weights = 1, except for first and last elements (-6 and +6 months) = 0.5, Normalization by 1/12 factor). This is the same smoothing as the standard smoothing applied to the total monthly sunspot numbers. There are no smoothed values for the first 6 months and last 6 months of the data series.Choice of smoothing: This 13-month smoothed series is provided only for backward compatibility with a large number of past publications and methods resting on this smoothed series. It has thus become a base standard (e.g., for the conventional definition of the times of minima and maxima of solar cycles). However, a wide range of other smoothing functions can be used, often with better low-pass filtering and anti-aliasing properties. As the optimal filter choice depends on the application, we thus invite users to start from the monthly mean Sunspot Numbers and apply the smoothing function that is most appropriate for their analyses. The classical smoothed series included here should only be used when direct comparisons with past published analyses must be made.

  Sunspot - ISN Monthly Smoothed - v2 (North)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Monthly smoothed mean Northern hemisphere sunspot numbers. The 13-month smoothed monthly sunspot numbers are derived by a tapered-boxcar running mean of monthly Northern hemisphere sunspot numbers over 13 months centered on the corresponding month (Smoothing function: equal weights = 1, except for first and last elements (-6 and +6 months) = 0.5, Normalization by 1/12 factor). This is the same smoothing as the standard smoothing applied to the total monthly sunspot numbers. There are no smoothed values for the first 6 months and last 6 months of the data series. Choice of smoothing: This 13-month smoothed series is provided only for backward compatibility with a large number of past publications and methods resting on this smoothed series. It has thus become a base standard (e.g., for the conventional definition of the times of minima and maxima of solar cycles). However, a wide range of other smoothing functions can be used, often with better low-pass filtering and anti-aliasing properties. As the optimal filter choice depends on the application, we thus invite users to start from the monthly mean Sunspot Numbers and apply the smoothing function that is most appropriate for their analyses. The classical smoothed series included here should only be used when direct comparisons with past published analyses must be made.

  Sunspot - ISN Monthly Smoothed - v2 (Total)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

The 13-month smoothed monthly sunspot number is derived by a tapered-boxcar running mean of monthly sunspot numbers over 13 months centered on the corresponding month (Smoothing function: equal weights = 1, except for first and last elements (-6 and +6 months) = 0.5, Normalization by 1/12 factor). There are no smoothed values for the first 6 months and last 6 months of the data series.Choice of smoothing: This 13-month smoothed series is provided only for backward compatibility with a large number of past publications and methods resting on this smoothed series. It has thus become a base standard (e.g., for the conventional definition of the times of minima and maxima of solar cycles). However, a wide range of other smoothing functions can be used, often with better low-pass filtering and anti-aliasing properties. As the optimal filter choice depends on the application, we thus invite users to start from the monthly mean Sunspot Numbers and apply the smoothing function that is most appropriate for their analyses. The classical smoothed series included here should only be used when direct comparisons with past published analyses must be made.

  Sunspot - ISN Monthly - v2 (South)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Monthly mean Southern hemisphere sunspot numbers obtained by taking a simple arithmetic mean of the daily Southern hemisphere sunspot numbers over all days of each calendar month. Each sunspot group is counted in the Southern hemisphere based on its heliographic latitude. NB: Southern hemisphere numbers are always normalized to the corresponding total monthly mean sunspot number.

  Sunspot - ISN Monthly - v2 (Total)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: monthly data
downsampled data: yearly data
raw data: monthly data
downsampled data: yearly data
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Monthly mean total sunspot number obtained by taking a simple arithmetic mean of the daily total sunspot number over all days of each calendar month. Monthly means are available only since 1749 because the original observations compiled by Rudolph Wolf were too sparse before that year. (Only yearly means are available back to 1700)

  Sunspot - ISN Yearly - v2 (Total)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: yearly data
downsampled data:
raw data: yearly data
downsampled data:
   
   
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Yearly mean total sunspot number obtained by taking a simple arithmetic mean of the daily total sunspot number over all days of each year. (NB: in early years in particular before 1749, the means are computed on only a fraction of the days in each year because on many days, no observation is available).

  Sunspot - ISN Monthly (Total) Forecast - v2 (Standard Curves)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Forecasts of the monthly mean sunspot number using the Standard Curve method (extension of the original method by M. Waldmeier). The method consists in the least-square fit and interpolation of a set of standard curves, each curve corresponding to the average shape of solar cycles of a narrow range of maximum value. The fit is done on the observed 13-month smoothed monthly sunspot number, using the last 24 available values. This is why the prediction actually starts 5 months before the last elapsed month and runs over 18 months (up to 12 months ahead). This method performs well in the middle of each cycle, but as all methods based purely on past solar activity, it becomes unreliable at the end of each cycle and during the minima.

  Sunspot - ISN Monthly (Total) Forecast - v2 (Combined Method)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Forecasts of the monthly mean sunspot number using the Combined Method. The base method consists in the least-square fit and interpolation over all past recorded cycles since 1749. The fit is done on the observed 13-month smoothed monthly sunspot number (all available values since either the last minimum or last maximum of the cycle). This is why the prediction actually starts 5 months before the last elapsed month and runs over 18 months (up to 12 months ahead). In order to obtain a reliable prediction around the time of cycle minima (from 1.5 year before to up to the next maximum), the fit uses the aa geomagnetic index as precursor index for predicting the maximum value of the next cycle. The least-square fit then uses a combination of the last observed monthly sunspot number and this aa-based prediction of the next maximum value (until it is actually reached).

Ref: K. Denkmayr, P. Cugnon, 1997 : About Sunspot Number Medium-Term Predictions, in Solar-Terrestrial Prediction Workshop V, eds. G.Heckman et al., Hiraiso Solar Terrestrial Research Center, Japan, p. 103.

  Sunspot - ISN Monthly (Total) Forecast - v2 (Improved Combined Method)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Improved 12-month ahead predictions obtained by applying an adaptative Kalman filter to the primary Combined Method (CM) predictions from WDC-SILSO. This technique improves the approximation of the smoothed monthly sunspot number over the last 6 months, i.e., the interval between the last available smoothed value of the sunspot number and the current month of the prediction.

(Ref.: T. Podladchikova, R. Van der Linden, 2011: A Kalman Filter Technique for Improving Medium-Term Predictions of the Sunspot Number. Solar Physics. DOI: 10.1007/s11207-011-9899-y)

  Sunspot - ISN Monthly (Total) Forecast - v2 (Improved McNish and Lincoln Method)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Kalman filter improvement of the monthly smoothed Sunspot Number prediction by McNish & Lincoln method (M&L). Predictions of M&L method were taken from ftp://ftp.ngdc.noaa.gov/STP/space-weather/solar-data/solar-indices/sunspot-numbers/predicted.

The improvement of the predictions is provided by applying an adaptive Kalman filter to obtained medium-term predictions using the last six monthly mean values of sunspot numbers, which cover the six months between the last available value of the 13-month running mean (the starting point for the predictions) and the current time. The proposed technique reduces stochastic component of the last six monthly mean sunspot numbers that give significant information about cycle evolution and provides effective estimate of sunspot activity at the current time. This estimate becomes the new starting point for the prediction updating that is shifted six month ahead in comparison with the last observed 13-month running mean and provides an increase of prediction accuracy for medium-term methods.

Correction technique was proposed by T. Podladchikova and R. Van der Linden and improves medium term prediction methods as they are monthly updated using the last available observations of smoothed sunspot numbers. ref.: T. Podladchikova, R. Van der Linden, 2011: A Kalman Filter Technique for Improving Medium-Term Predictions of the Sunspot Number. Solar Physics.

  Sunspot - ISN Monthly (Total) Forecast - v2 (Improved Standard Method)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information:

Improved 12-month ahead predictions obtained by applying an adaptative Kalman filter to the primary Standard Curve (SC) prodictions from WDC-SILSO. This technique improves the approximation of the smoothed monthly sunspot number over the last 6 months, i.e., the interval between the last available smoothed value of the sunspot number and the current month of the prediction.

(Ref.: T. Podladchikova, R. Van der Linden, 2011: A Kalman Filter Technique for Improving Medium-Term Predictions of the Sunspot Number. Solar Physics. DOI: 10.1007/s11207-011-9899-y)

  Sunspot - ISN Monthly (Total) Forecast - v2 (McNish And Lincoln Method)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: SILSO
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
  raw data: monthly data
downsampled data: yearly data
  
    
Source Location: Ground Based
Units:
Import latency: 360 + ~5 minutes.
Information: Forecasts of the monthly mean sunspot number using the McNish and Lincoln method. The base principle was described in McNish A.G. & Lincoln J.V. 1949, (Trans. Am. Geophys. Union 30, 673-685). The method was further refined in the mid-1970s by J.V. Lincoln (no published documentation), to include the latest solar cycles and to use monthly means instead of yearly means. These were the standard solar cycle predictions provided until recently by the SWPC-NOAA. Based on the original Fortran code kindly provided by the NCEI (NOAA, Boulder, USA), we reprogrammed the calculation in a modern form, while documenting this implementation. This method consists in least-square fitting a single mean cycle profile to the last 13-month smoothed sunspot number. This mean cycle is obtained by a simple averaging of all cycles between 1849 and 1975 (cycles 9 to 20), aligned on the time of their preceding minimum. This method can provide a reasonable prediction in the course of a cycle and a fair estimate of the upcoming maximum in the rising phase of the cycle. On the other hand, it is unusable around the times of cycle minima (+/- 1.5 year) and cannot provide any prediction of the expected length of a cycle (cf. Hildner, E. and Greer M.S, 1990, in R. I. Thompson, D. Cole, P. J. Wilkinson, M. A. Shea, and G. Heckman (eds.), Proceedings of Solar-Terrestrial Prediction Workshop III , NOAA and AFGL, USA. )

  Radio - 10.7 cm flux (Observed)


Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
 raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
 1 day prediction2 days prediction3 days prediction
Source Location: Ground Based
Units: sfu (Solar Flux Units)
Import latency: 60 + ~5 minutes.
Information: The F10.7 index is a measure of the solar radio flux per unit frequency at a wavelength of 10.7 cm, near the peak of the observed solar radio emission. F10.7 is often expressed in SFU or solar flux units (1 SFU = 10-22 W m-2 Hz-1). It represents a measure of diffuse, nonradiative heating of the coronal plasma trapped by magnetic fields over Active Regions. It is an excellent indicator of overall solar activity levels and correlates well with solar UV emissions. The F10.7 index is measured daily at local noon in a bandwidth of 100 MHz centered on 2800 MHz at the Penticton site of the Dominion Radio Astrophysical Observatory (DRAO), Canada. The F10.7 (Observed) values represented in STAFF have not been adjusted to 1 AU. The solar F10.7 cm record extends back to 1947, and is the longest direct record of solar activity available, other than sunspot-related quantities. Prediction 1, 2 and 3 are the predicted values of the F10.7 index that SIDC forecasters predict with one, two and three days lead time respectively.

  Radio - 10.7 cm flux (Adjusted)


Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Ground Based
Units: sfu (Solar Flux Units)
Import latency: 60 + ~5 minutes.
Information: The Adjusted F10.7 cm flux index is a measure of the solar radio flux per unit frequency at a wavelength of 10.7 cm, near the peak of the observed solar radio emission. F10.7 is often expressed in SFU or solar flux units (1 SFU = 10-22 W m-2 Hz-1). It represents a measure of diffuse, nonradiative heating of the coronal plasma trapped by magnetic fields over Active Regions. It is an excellent indicator of overall solar activity levels and correlates well with solar UV emissions. The F10.7 index is measured daily at local noon in a bandwidth of 100 MHz centered on 2800 MHz at the Penticton site of the Dominion Radio Astrophysical Observatory (DRAO), Canada. The F10.7 (Adjusted) values represented in STAFF have been adjusted to 1 AU. The solar F10.7 cm record extends back to 1947, and is the longest direct record of solar activity available, other than sunspot-related quantities.

  Particles - ACE SIS Particles at > 10 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 10 MeV or larger, as measured by the SIS instrument onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  Particles - ACE SIS Particles at > 30 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 30 MeV or larger, as measured by the SIS instrument onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  Particles - GOES Electrons at > 0.8 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 0.8 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Electrons at > 0.8 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 0.8 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Electrons at > 2.0 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 2.0 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Electrons at > 2.0 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 2.0 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Electrons at > 4.0 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 4.0 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Electrons at > 4.0 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of electrons with an energy of 4.0 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 1 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 1 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 10 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 10 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 100 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 100 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 100 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 100 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 10 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 10 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 1 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 1 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 30 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 30 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 30 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 30 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 5 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 5 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 50 Mev


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 50 MeV or larger, as measured by the primary SWPC GOES satellite.

  Particles - GOES Particles at > 50 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 50 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - GOES Particles at > 5 Mev (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: Count/(cm^2 s sr)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the flux of particles with an energy of 5 MeV or larger, as measured by the secondary SWPC GOES satellite.

  Particles - STEREO A CNO Flux (HET, 30-52 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of CNO particles with an energy between 30 and 52 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A CNO Flux (HET, 52-74 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of CNO particles with an energy between 52 and 74 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A Electron Flux (HET, 0.7-4.0 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of electrons with an energy between 0.7 and 4.0 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A Fe Flux (HET, 52-74 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of Fe nuclei with an energy between 52 and 74 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A He Flux (HET, 13-21 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 13 and 21 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A He Flux (HET, 21-40 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 21 and 40 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A He Flux (HET, 40-100 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 40 and 100 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A Proton Flux (HET, 13-21 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 13 and 21 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A Proton Flux (HET, 21-40 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 21 and 40 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO A Proton Flux (HET, 40-100 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 40 and 100 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B CNO Flux (HET, 30-52 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of CNO particles with an energy between 30 and 52 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B CNO Flux (HET, 52-74 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of CNO particles with an energy between 52 and 74 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B Electron Flux (HET, 0.7-4.0 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of electrons with an energy between 0.7 and 4.0 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B Fe Flux (HET, 52-74 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of Fe nuclei with an energy between 52 and 74 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B He Flux (HET, 13-21 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 13 and 21 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B He Flux (HET, 21-40 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 21 and 40 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B He Flux (HET, 40-100 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of He nuclei with an energy between 40 and 100 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B Proton Flux (HET, 13-21 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 13 and 21 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B Proton Flux (HET, 21-40 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 21 and 40 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Particles - STEREO B Proton Flux (HET, 40-100 MeV)


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location:
Units: Count/(cm^2 s sr MeV)
Import latency: 5 + ~5 minutes.
Information: This timeline provides the HET differential flux of protons with an energy between 40 and 100 MeV, as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - ACE Solar Wind Density


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind proton density as measured by the SWEPAM instrument (Solar Wind Electron Proton Alpha Monitor) onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  Solar Wind - ACE Solar Wind Speed


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: km/s
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind speed as measured by the SWEPAM instrument (Solar Wind Electron Proton Alpha Monitor) onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  Solar Wind - ACE Solar Wind Temperature


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: K
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind ion temperature as measured by the SWEPAM instrument (Solar Wind Electron Proton Alpha Monitor) onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  Solar Wind - DSCOVR Solar Wind Density


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the solar wind proton density (in protons per cm3) as measured by the Faraday Cup (FC) onboard the DSCOVR satellite near the L1 point.

  Solar Wind - DSCOVR Solar Wind Speed


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: km/s
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the solar wind proton bulk speed (in km/s) as measured by the Faraday Cup (FC) onboard the DSCOVR satellite near the L1 point.

  Solar Wind - DSCOVR Solar Wind Temperature


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: K
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the solar wind proton temperature (in K) as measured by the Faraday Cup (FC) onboard the DSCOVR satellite near the L1 point.

  Solar Wind - Soho Celias Solar Wind Arrival Direction


Institution:University of Maryland University of Maryland
Division: 
Predictions provider: CELIAS/MTOF Proton Monitor
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: Degrees
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the flow direction of the solar wind (in degrees) in the plane perpendicular to the ecliptic plane, with positive values indicating flow FROM the South, as measured by the MTOF Proton Monitor onboard SOHO. On rare occasions the spacecrafts roll angle is changed for brief periods, during which the derived flow direction will refer to a different plane. A list of such times is available.

  Solar Wind - Soho Celias Solar Wind Density


Institution:University of Maryland University of Maryland
Division: 
Predictions provider: CELIAS/MTOF Proton Monitor
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the solar wind proton density (in protons per cm3) as measured by the MTOF Proton Monitor onboard SOHO.

  Solar Wind - Soho Celias Solar Wind Speed


Institution:University of Maryland University of Maryland
Division: 
Predictions provider: CELIAS/MTOF Proton Monitor
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: km/s
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the solar wind proton bulk speed (in kilometers per second) as measured by the MTOF Proton Monitor onboard SOHO.

  Solar Wind - Soho Celias Solar Wind Thermal Speed


Institution:University of Maryland University of Maryland
Division: 
Predictions provider: CELIAS/MTOF Proton Monitor
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: km/s
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the most probable thermal speed of the solar wind protons (in kilometers per second) as measured by the MTOF Proton Monitor onboard SOHO. This thermal speed is calculated as Sqrt(2kT/m).

  Solar Wind - Stereo A Solar Wind Density


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind proton density as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - Stereo A Solar Wind Speed


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: km/s
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind speed as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - Stereo A Solar Wind Temperature


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: K
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind ion temperature as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - Stereo B Solar Wind Density


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind proton density as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - Stereo B Solar Wind Speed


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: km/s
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind speed as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - Stereo B Solar Wind Temperature


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: K
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind ion temperature as measured by the PLASTIC instrument (PLAsma and SupraThermal Ion Composition) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  Solar Wind - WIND Solar Wind Density


Institution:NASA NASA
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: Count/cc
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind proton density as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

(Data source OMNIWeb)

  Solar Wind - WIND Solar Wind Speed


Institution:NASA NASA
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: km/s
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind speed as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

(Data source OMNIWeb)

  Solar Wind - WIND Solar Wind Temperature


Institution:NASA NASA
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: K
Import latency: 5 + ~5 minutes.
Information: This timeline provides the solar wind temperature as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

(Data source OMNIWeb)

  IMF - ACE IMF Bt


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the magnitude of the Interplanetary Magnetic Field (B vector) as measured by the MAG magnetometer onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  IMF - ACE IMF Bx


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the x-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  IMF - ACE IMF By


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the y-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  IMF - ACE IMF Bz


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the z-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the Advanced Composition Explorer (ACE) satellite near the L1 point.

  IMF - ACE IMF Phi


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location: L1
Units: Degrees
Import latency: 5 + ~5 minutes.
Information: This timeline provides the phi angle of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the Advanced Composition Explorer (ACE) satellite near the L1 point. This is the angle (seen from the Earth) between the Sun and the IMF B vector.

  IMF - DSCOVR IMF Bt


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information:

This timeline provides the magnitude of the Interplanetary Magnetic Field (B vector) as measured by the MAG magnetometer onboard the DSCOVR satellite near the L1 point.

  IMF - DSCOVR IMF Bx


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the x-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the DSCOVR satellite near the L1 point.

  IMF - DSCOVR IMF By


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the y-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the DSCOVR satellite near the L1 point.

  IMF - DSCOVR IMF Bz


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the z-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the DSCOVR satellite near the L1 point.

  IMF - DSCOVR IMF Phi


Institution:NOAA NOAA
Division: SWPC
Predictions provider: DSCOVR
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: L1
Units: Degrees
Import latency: 5 + ~5 minutes.
Information: This timeline provides the phi angle of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the MAG magnetometer onboard the DSCOVR satellite near the L1 point. This is the angle between the Sun and the IMF B vector.

  IMF - STEREO A IMF Bt


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the magnitude of the Interplanetary Magnetic Field (B vector) as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO A IMF Bx


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the x-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO A IMF By


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the y-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO A IMF Bz


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the z-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory A (STEREO A) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO B IMF Bt


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the magnitude of the Interplanetary Magnetic Field (B vector) as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO B IMF Bx


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the x-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO B IMF By


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the y-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - STEREO B IMF Bz


Institution:NASA NASA
Division: STEREO Science Center
Predictions provider: STEREO Science Center
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
   
Source Location:
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the z-component of the Interplanetary Magnetic Field (B vector) in the HGRTN coordinate frame as measured by the IMPACT instrument (In-situ Measurements of Particles and CME Transients) onboard the Solar Terrestrial Relations Observatory B (STEREO B) satellite which orbits the Sun at roughly the same distance as the Earth (see https://stereo-ssc.nascom.nasa.gov/where.shtml).

  IMF - WIND IMF Bt


Institution:NASA NASA
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the magnitude of the Interplanetary Magnetic Field (B vector) as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

(Data source OMNIWeb)

  IMF - WIND IMF Bx


Institution:NASA NASA
Division: 
Predictions provider: OMNIWEB
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the x-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

  IMF - WIND IMF By


Institution:NASA NASA
Division: 
Predictions provider: OMNIWEB
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the y-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

  IMF - WIND IMF Bz


Institution:NASA NASA
Division: 
Predictions provider: OMNIWEB
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the z-component of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point.

  IMF - WIND IMF Phi


Institution:NASA NASA
Division: 
Predictions provider: OMNIWEB
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: L1
Units: Degrees
Import latency: 5 + ~5 minutes.
Information: This timeline provides the phi angle of the Interplanetary Magnetic Field (B vector) in the GSM coordinate frame as measured by the Global Geospace Science (GGS) WIND satellite near the L1 point. This is the angle (seen from the Earth) between the Sun and the IMF B vector.

  Geomagnetic - Ak (Chambon-La-Forêt)


Institution:Observatoire magnétique de Chambon-la-Forêt
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: daily
downsampled data: 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the geomagnetic Ak index measured at the Observatoire magnétique de Chambon-la-Forêt, France.

  Geomagnetic - Ap (Potsdam)


Institution:Helmholtz Center Potsdam Helmholtz Center Potsdam
Division: 
Predictions provider: Space Research Institute, Kyiv, Ukraine
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 3 hour data   
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the official geomagnetic (planetary) Ap index calculated by the Helmholtz Center Potsdam.

  Geomagnetic - Dst


Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
 1 hour prediction2 hour prediction3 hour prediction
Source Location: Ground Based
Units: nT
Import latency: 5 + ~5 minutes.
Information: This timeline provides the official Dst values calculated by the World Data Center for Geomagnetism, Kyoto (WDC-C2). Prediction 1, 2 and 3 are the predicted values with one, two and three hour lead time respectively of Dst as predicted by the geomagnetic forecast module developed within the AFFECTS FP7 project at the Space Research Institute, Kyiv, Ukraine.

  Geomagnetic - GOES Magnetometer (He)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (He) (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (Hn)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (Hn) (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (Hp)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations.

  Geomagnetic - GOES Magnetometer (Hp) (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (Total)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - GOES Magnetometer (Total) (Secondary)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: 1 minute data
downsampled data: 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
   
    
Source Location: GEO
Units: nT
Import latency: 5 + ~5 minutes.
Information: Since 1975, each of NOAAs Geostationary Operational Environmental Satellites (GOES), located in Earths geographic equatorial plane, approximately 6.6 Earth radii from the center of Earth, have carried magnetometers to monitor the geomagnetic field and its variations. Typically there are two GOES operational satellites: GOES East, located over the east coast of the U.S. and GOES West, located over the Pacific, just west of the U.S. mainland. At times, though, data are available from more than the two prime operational satellites. The geomagnetic field measurements are important for interpreting GOES energetic particle measurements and for providing alerts to many customers, specifically for indicating the onset of a geomagnetic storm (known as a sudden storm commencement). GOES magnetometer data have been used for constructing magnetic field models, and to help forecasters identify the buildup and release of energy in Earths magnetosphere that occurs during geomagnetic storms and substorms. The magnetic field measurements can also indicate when the solar wind has pushed the boundary of the magnetosphere, the magnetopause, inside of geosynchronous orbit. Those situations are usually during very disturbed space weather conditions and can be important for spacecraft operations. GOES Magnetometer data are also important in research, being among the most widely used spacecraft data by the national and international solar and space weather research community (see e.g. NASA CDAWeb usage statistics). The data have often been used to support launch decisions for research sounding rockets. The measurements can also be used to validate large-scale space environment models of the coupled magnetosphere and ionosphere.

  Geomagnetic - K (Chambon-La-Forêt)


Institution:Observatoire magnétique de Chambon-la-Forêt
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 3 hour data   
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the geomagnetic K index measured at the Observatoire magnétique de Chambon-la-Forêt, France.

  Geomagnetic - K (Dourbes)


Institution:Royal Meteorological Institute of Belgium Royal Meteorological Institute of Belgium
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 3 hour data   
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the geomagnetic K index measured at the Geophysical Center of Dourbes, Belgium.

  Geomagnetic - Kp (NOAA)


Institution:NOAA NOAA
Division: SWPC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 3 hour data   
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the estimated geomagnetic (planetary) Kp index calculated by NOAA/SWPC. It is available in near real time but generally contains information from less stations than the official Kp of Potsdam.

  Geomagnetic - Kp (Potsdam)


Institution:Helmholtz Center Potsdam Helmholtz Center Potsdam
Division: 
Predictions provider: Space Research Institute, Kyiv, Ukraine
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
  
 3 hour data3 hour prediction  
Source Location: Ground Based
Units:
Import latency: 5 + ~5 minutes.
Information: This timeline provides the official geomagnetic (planetary) Kp index calculated by the Helmholtz Center Potsdam. Prediction 1 is the predicted value with one hour lead time of Kp (Potsdam) as predicted by the geomagnetic forecast module developed within the AFFECTS FP7 project at the Space Research Institute, Kyiv, Ukraine.

  Ionosphere - SIMONE


Institution:Gymnasium Walsrode Gymnasium Walsrode
Division: 
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 5 second data
downsampled data: 1 minute data, 5 minute data, hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
    
Source Location: Ground Based
Units: V
Import latency: 15 + ~5 minutes.
Information:

SIMONE (Sonnen und Ionosphären MOnitoring NEtzwerk) is an SID Monitor (SIDMON): an earth-bound space weather monitor which measures the effects on earth-ionosphere of solar flares by tracking changes in very low frequency (VLF) transmissions as they propagate from the transmitter to the receiver through the earth-ionosphere-waveguide. The VLF radio waves induce the antenna with small voltages, becoming intensified by the SIDMON, digitized and recorded in a CSV-file in a PC.

The SIDMON works like a radio receiver for a special frequency and is tuned to very low frequencies. The SIMONE SIDMON with monitor ID S-0082 is tuned to 24 kHz, that is the VLF frequency of the transmitter NAA in Cutler, USA. A self made antenna (ca. 187 m, frame of 1.25m x 1.25 m, 37 coils) picks up this analog VLF signal and the RG-58 Coax cable connects the antenna to the SIDMON (BNC connector). A DataQ A/D converter is plugged into the SIDMON and an RS-232 cable connects the DataQ with the computer, there is a special software installed (SIDMON CD). The output is an uncalibrated voltage, tuned to the interval [-5 V, +5 V]. More information can be found in SID_TechManual_Rev1b.pdf.

SIMONE is hosted by and located at the Gymnasium Walsrode, Sunderstrasse 19, D 29664 Walsrode, Germany¬ (longitude 9.58 E, latitude 52.87 N). The location of the antenna and of the other part of the equipment was not changed between 2008-06-05 (first dataset) and 2013-06-04 (interruption between ˜18:00 UT until ˜19:00 UT and new adjustment). The distance between the new and old place is about 15 m, it is located in the top floor of the same building.

The SIDMON project was Developed at Stanford University under funding from the Center for Integrated Space Weather Modeling (CISM), a National Science Foundation (NSF) Science and Technology Center. Supported by NASAs Solar and Heliophysical Observatory/MDI consortium. SOHO is a project of international cooperation between ESA and NASA. Additional support from NASAs Solar Dynamics Observatory/HMI consortium. Credits and Acknowledgements: Stanford Solar Center, Deborah Scherrer, Project Lead. The High School Gymnasium Walsrode is involved in SIMONE as part of the international SID project led by the University of Stanford, in the framework of the UN International Space Weather Initiative, following the UN International Heliospheric Year (IHY) campaign. The project at Gymansium Walsrode is led by Mrs. Barbara Bernert in cooperation with Dr. Volker Bothmer at University Göttingen as SIMONE project lead.

  Ionosphere - VTEC - Vertical Electron Content (ROB, Brussels)


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: GNSS Research Group
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: 5 minute data
downsampled data: hourly data, daily, 1 carrington rotation data, monthly data, yearly data
    
15 minutes data    
Source Location: Ground Based
Units: tecu (1e16 electrons/m2)
Import latency: 15 + ~5 minutes.
Information: This timeline provides the VTEC (Vertical Electron Content) over Brussels, as estimated from EUREF Permanent Network (EPN) GPS data by the GNSS Research Group at the Royal Observatory of Brussels.

  EIT 171 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  EIT 171 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  EIT 171 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  EIT 171 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  EIT 171 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 171 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  EIT 171 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  EIT 195 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  EIT 195 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  EIT 195 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  EIT 195 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  EIT 195 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  EIT 195 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  EIT 195 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 94 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 94 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 94 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 94 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 94 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 94 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 94 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 94 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 131 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 131 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 131 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 131 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 131 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 131 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 131 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 131 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 171 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 171 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 171 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 171 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 171 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 171 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 171 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 193 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 193 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 193 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 193 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 193 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 193 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 193 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 211 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 211 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 211 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 211 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 211 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 211 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 211 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 211 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 304 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 304 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 304 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 304 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 304 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 304 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 304 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 304 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 335 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 335 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 335 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 335 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 335 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 335 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 335 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 335 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 1600 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 1600 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 1600 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 1600 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 1600 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1600 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 1600 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1600 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 1700 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 1700 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 1700 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 1700 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 1700 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 1700 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 1700 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 1700 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  AIA 4500 Stats - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the maximal pixel intensity in the corresponding EUV image.

  AIA 4500 Stats - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the mean pixel intensity in the corresponding EUV image.

  AIA 4500 Stats - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the median pixel intensity in the corresponding EUV image.

  AIA 4500 Stats - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the minimal pixel intensity in the corresponding EUV image.

  AIA 4500 Stats - On Disk - Maximum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the maximal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - On Disk - Mean Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the mean pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the median pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - On Disk - Minimum Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the minimal pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - On Disk - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the total pixel intensity in the on-disk part of the corresponding EUV image.

  AIA 4500 Stats - Standard Deviation


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the standard deviation of the intensity in the corresponding EUV image.

  AIA 4500 Stats - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
 raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
 6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 4500 Angstrom). A data point of this timeline provides the total pixel intensity in the corresponding EUV image.

  SPoCA EIT 171 - Active Regions - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Active Regions On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Coronal Holes Central Meridian - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Coronal Holes On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Coronal Holes On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Coronal Holes On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Coronal Holes On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Quiet Sun On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Quiet Sun On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Quiet Sun On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 171 - Quiet Sun On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Active Regions On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Coronal Holes Central Meridian - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Coronal Holes On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Coronal Holes On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Coronal Holes On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Coronal Holes On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Quiet Sun On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Quiet Sun On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Quiet Sun On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA EIT 195 - Quiet Sun On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
    
6 hour data    
Source Location: L1
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SOHO/EIT 195 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Active Regions On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Coronal Holes Central Meridian - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Coronal Holes On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Coronal Holes On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Coronal Holes On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Coronal Holes On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Quiet Sun On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Quiet Sun On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Quiet Sun On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 171 - Quiet Sun On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 180 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 171 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Active Regions On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Coronal Holes Central Meridian - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Coronal Holes On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Coronal Holes On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Coronal Holes On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Coronal Holes On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Quiet Sun On Disk - Raw Area


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: Mm^2
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Quiet Sun On Disk - Filling Factor


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units:
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Quiet Sun On Disk - Median Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.

  SPoCA AIA 193 - Quiet Sun On Disk - Total Intensity


Institution:Royal Observatory of Belgium Royal Observatory of Belgium
Division: SIDC
Predictions provider: 
Precision & Downsampling
ScienceQuicklookPredictions 1Predictions 2Predictions 3
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
raw data: hourly data
downsampled data: daily, 1 carrington rotation data, monthly data, yearly data
   
6 hour data6 hour data   
Source Location: GEO
Units: DN/s
Import latency: 0 + ~5 minutes.
Information: Each data point of this timeline corresponds to an EUV image (SDO/AIA 193 Angstrom). The SPoCA algorithm (Verbeeck et al. 2014, A&A, 561, A29) was employed to segment the EUV image into Active Regions, Coronal Holes, and Quiet Sun (on-disk and off-disk). A data point of this timeline provides the total raw area of all Active Regions as measured in the plane of the corresponding EUV image.