In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 125, No. 9 ( 2020-09)
Abstract:
Solar cycle phase lags between energetic proton fluxes and sunspot number depend on solar cycle, L m , B / B 0 , and proton energy The ratios of the maximal to minimal values of 〉 16‐MeV proton fluxes at the same location from 1978 to 2014 depend on L m and B / B 0 as well An exponential equation with an offset for the relationship between log 10 (proton flux) and F10.7 flux can improve the NOAAPRO model
Type of Medium:
Online Resource
ISSN:
2169-9380
,
2169-9402
DOI:
10.1029/2019JA027635
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2020
detail.hit.zdb_id:
2033040-6
detail.hit.zdb_id:
161665-1
detail.hit.zdb_id:
3094181-7
SSG:
16,13
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