Welcome to STAFF

Solar Timelines viewer for AFFects
AFFECTS FP7 Royal Observatory of Belgium Solar-Terrestrial Centre of Excellence
 

Dataset Selection

GOES X-Ray flux 0.1-0.8 nm
GOES X-Ray flux 0.05-0.4 nm
Lyra Lyman Alpha
Lyra Aluminium
Lyra Herzberg
Lyra Zirconium
ISN Daily (North)
ISN Daily (South)
ISN Daily (Total)
ISN Monthly (North)
ISN Monthly Smoothed (North)
ISN Monthly Smoothed (South)
ISN Monthly Smoothed (Total)
ISN Monthly (South)
ISN Monthly (Total)
ISN Yearly (Total)
ISN Monthly (Total) Forecast (Combined Method)
ISN Monthly (Total) Forecast (Improved Combined Method)
ISN Monthly (Total) Forecast (Improved McNish And Lincoln Method)
ISN Monthly (Total) Forecast (Improved Standard Method)
ISN Monthly (Total) Forecast (Standard Curves)
10.7 cm flux
GOES Electrons at > 0.8 Mev
GOES Electrons at > 2.0 Mev
GOES Particles at > 1 Mev
GOES Particles at > 10 Mev
GOES Particles at > 100 Mev
GOES Particles at > 30 Mev
GOES Particles at > 5 Mev
GOES Particles at > 50 Mev
ACE Solar Wind Density
ACE Solar Wind Speed
ACE Solar Wind Temperature
WIND Solar Wind Density
WIND Solar Wind Speed
WIND Solar Wind Temperature
ACE IMF Bt
ACE IMF Bx
ACE IMF By
ACE IMF Bz
ACE IMF Phi
WIND IMF Bt
WIND IMF Bx
WIND IMF By
WIND IMF Bz
WIND IMF Phi
Ak (Chambon-La-Forêt)
Ap (Potsdam)
Dst
K (Chambon-La-Forêt)
K (Dourbes)
Kp (NOAA)
Kp (Potsdam)
SIMONE
VTEC - Vertical Electron Content (ROB, Brussels)
Active Regions - Raw Area
Active Regions - Median Intensity
Active Regions - Total Intensity
Active Regions On Disk - Raw Area
Active Regions On Disk - Filling Factor
Active Regions On Disk - Median Intensity
Active Regions On Disk - Total Intensity
Coronal Holes Central Meridian - Filling Factor
Coronal Holes On Disk - Raw Area
Coronal Holes On Disk - Filling Factor
Coronal Holes On Disk - Median Intensity
Coronal Holes On Disk - Total Intensity
Quiet Sun On Disk - Raw Area
Quiet Sun On Disk - Filling Factor
Quiet Sun On Disk - Median Intensity
Quiet Sun On Disk - Total Intensity
Active Regions - Raw Area
Active Regions - Median Intensity
Active Regions - Total Intensity
Active Regions On Disk - Raw Area
Active Regions On Disk - Filling Factor
Active Regions On Disk - Median Intensity
Active Regions On Disk - Total Intensity
Coronal Holes Central Meridian - Filling Factor
Coronal Holes On Disk - Raw Area
Coronal Holes On Disk - Filling Factor
Coronal Holes On Disk - Median Intensity
Coronal Holes On Disk - Total Intensity
Quiet Sun On Disk - Raw Area
Quiet Sun On Disk - Filling Factor
Quiet Sun On Disk - Median Intensity
Quiet Sun On Disk - Total Intensity
Active Regions - Raw Area
Active Regions - Median Intensity
Active Regions - Total Intensity
Active Regions On Disk - Raw Area
Active Regions On Disk - Filling Factor
Active Regions On Disk - Median Intensity
Active Regions On Disk - Total Intensity
Coronal Holes Central Meridian - Filling Factor
Coronal Holes On Disk - Raw Area
Coronal Holes On Disk - Filling Factor
Coronal Holes On Disk - Median Intensity
Coronal Holes On Disk - Total Intensity
Quiet Sun On Disk - Raw Area
Quiet Sun On Disk - Filling Factor
Quiet Sun On Disk - Median Intensity
Quiet Sun On Disk - Total Intensity
Active Regions - Raw Area
Active Regions - Median Intensity
Active Regions - Total Intensity
Active Regions On Disk - Raw Area
Active Regions On Disk - Filling Factor
Active Regions On Disk - Median Intensity
Active Regions On Disk - Total Intensity
Coronal Holes Central Meridian - Filling Factor
Coronal Holes On Disk - Raw Area
Coronal Holes On Disk - Filling Factor
Coronal Holes On Disk - Median Intensity
Coronal Holes On Disk - Total Intensity
Quiet Sun On Disk - Raw Area
Quiet Sun On Disk - Filling Factor
Quiet Sun On Disk - Median Intensity
Quiet Sun On Disk - Total Intensity
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STAFF
STAFF - Solar Timelines viewer for Affects
Version: 5.0
Why?

Staff is developed to allow a user easy access to huge amounts of timeline data.

What?

With a few clicks the user can see different types of plots even simultaneously if desired.
With the power of Staff, the user can effectively use it for Space Weather Forecasting, data analysis, publication and correlations between different types of data. In addition the data can be exported to image or data file for further usage.

How?

Staff is developed with Java, html and javascript technology on top of a PostGreSql database. Due to the downsampling of the data, the load time of the website is fast and clean, in addition, the site uses little parameters and only sends postbacks when absolutely necessary allowing pleasant user interaction.

Where?

Application is developed and data resides @ Royal Observatory Belgium.

When?

Never and always, Staff is continuously updated.

Who?

Staff was developed by Vincent Malisse (Royal Observatory of Belgium).
The concept comes from Dr. Cis Verbeeck (Royal Observatory of Belgium).

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Axes Labels Color:
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X-Ray

Copy the xml parameters in the textbox and press OK.

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Press the create button to create the xml and copy/paste the generated value.

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