Image Details
Caption: Figure 2.
Panel (a): percentage of the flux variation of the solar extended component above 250 MeV, 500 MeV, and 1 GeV vs. time. For normalization, the average flux values used are 30.00, 13.99, and 5.95 (× 10−8 cm−2 s−1), respectively. The gray region defines systematic uncertainties. Panel (b): flux variation of the solar extended component above 1 GeV compared with the SSN. Panel (c): flux variation of the solar extended component above 1 GeV compared with the CR electron flux at 1.00–1.71 GV (M. Aguilar et al. 2023). Panel (d): flux variation of the solar extended component above 1 GeV compared with the flux variation of the disk component above 1 GeV.
© 2025. The Author(s). Published by the American Astronomical Society.