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
โฆ LIBER โฆ
Solar-cycle dependence of galactic cosmic ray flux
โ Scribed by G. D. Parker; R. L. Chasson; R. T. Hansen; S. F. Hansen
- Publisher
- Springer
- Year
- 1976
- Tongue
- English
- Weight
- 659 KB
- Volume
- 48
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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