Variations in EUV Irradiance: Comparison between LYRA, ESP, and SWAP Integrated Flux
Figure 5
SWAVINT data variation (b) and LYRA level 3 channel 2–4 data variation (a) in July 2010 with calibration campaign data (grey bands) and special campaign data (orange bands) indicated. The other downward spikes are a result of the stabilization effect after the spacecraft off-pointings required by the SWAP calibration campaigns.
