Quasi real-time view of the solar atmosphere from SDO/AIA and SOHO/LASCO.
EUV full-disk imagery of the solar corona.
Full-disk magnetogram of the solar photosphere.
MGN coronagraphic observations.
NRGF coronagraphic observations.
Combined EUV and coronagraphic view for CME tracking.
Coronagraphic view from GOES platform instruments.
The input data are sequences of visible-light coronagraphic images from SOHO/LASCO-C2 and EUV full-disk images from SDO/AIA (193 Å channel). LASCO data are calibrated and background-subtracted, enhanced using the NRGF filter (SunPy). AIA images are processed and enhanced with standard SunPy routines. Each movie covers 24 hours of solar activity and is updated every 6 hours.