Analysis of the 5303 ~ coronal line intensity and of the sunspot activity during the period 1962-1970 confirms the existence of two distinct maxima of solar activity, in accordance with the previous findings of Gnevyshev for the period 1954-1960.
โฆ LIBER โฆ
Evidence for an ultra-long cycle of solar activity
โ Scribed by R. Henkel
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 93 KB
- Volume
- 25
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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