Abstract
Analysis of the 5303 Å 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.
Original language | English |
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Pages (from-to) | 493-497 |
Number of pages | 5 |
Journal | Solar Physics |
Volume | 25 |
Issue number | 2 |
DOIs | |
State | Published - Aug 1972 |