Variations in EUV Irradiance: Comparison between LYRA, ESP, and SWAP Integrated Flux
Figure 6
LYRA level 3 channel 2–4 and ESP level 1 data variations (at combined responses of the channels QD and 18, and separately) in July 2010. The downward spikes in the ESP data on July 14, 2010 are due to the calibration maneuvers of SDO.
