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Origin of the solar-magnetic-cycle dependent semiannual variation in galactic cosmic-ray flux

โœ Scribed by Levy, E. H.

Book ID
119705268
Publisher
American Geophysical Union
Year
1978
Tongue
English
Weight
313 KB
Volume
5
Category
Article
ISSN
1944-8007

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The coronal green line intensity is inappropriate for correlation studies of galactic cosmic ray variations. Being a non-monotonic function of coronal temperature, the green line intensity is a good index of neither coronal temperature nor solar wind speed. A more appropriate measure of coronal acti