The voltages and currents are shown in the left part, the right part contains the present temperatures. The lower right part shows that the WIC and SI doors are open now. The other image shows sun sensor readings. The satellite is spinning at about 2.1 rpm and we see 4 sun readings in 2 minutes. All currents and voltages are nominally.
All systems work nominally.
The Wideband Imaging Camera WIC to image the aurora in broad band for maximum spatial resolution day and night. The Spectrographic Imager SI to measure different types of aurora and separating them by wavelength and to measure proton induced aurora by removing the bright geocorona emissions. Geocorona photometers GEO to observe the distribution of the geocorona emissions to derive the magnetospheric hydrogen content responsible for neutral atom generation in the magnetosphere. This enables the GEO photometers to perform a complete 360 degrees measurement during one rotation but the imagers have to compensate the apparent motion of the imaged Earth with the TDI technique. If you want to contact the team members by surface mail, email, or see the personal webpages, just visit the team page .