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Galactic cosmic ray modulation for sunspot cycle 23

✍ Scribed by H.S. Ahluwalia; C. Lopate; R.C. Ygbuhay; M.L. Duldig

Book ID: 108066314
Publisher: Elsevier Science
Year: 2010
Tongue: English
Weight: 396 KB
Volume: 46
Category: Article
ISSN: 0273-1177
DOI: 10.1016/j.asr.2010.04.008

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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