๐”– Bobbio Scriptorium
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Galactic cosmic ray flux simulation and prediction

โœ Scribed by R.A Nymmik; M.I Panasyuk; A.A Suslov


Publisher
Elsevier Science
Year
1996
Tongue
English
Weight
899 KB
Volume
17
Category
Article
ISSN
0273-1177

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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