Variations in EUV Irradiance: Comparison between LYRA, ESP, and SWAP Integrated Flux
Figure 9
LYRA level 1 data measured by all four channels of unit 2, measured and simulated SWAVINT, and simulated AIA average intensity variations during the second transit of the Moon (a) together with certain SWAP images taken during the second transit of the Moon (b) whose times of observation are indicated in vertical lines on the graphs.
