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Solar Physics

, Volume 20, Issue 2, pp 332–344 | Cite as

The asymmetry of solar activity in the years 1959–1969

  • M. Waldmeier
Article

Abstract

One of the most outstanding feature of solar activity in the decade 1959–1969 was a very strong asymmetry on the two hemispheres. On the northern hemisphere spots, faculae and prominences were more numerous and the white light corona was brighter than on the southern hemisphere. This happened as well in the main zone as in the polar zone. The green coronal line too was brighter on the northern hemisphere, but the intensity of the red line was asymmetric in the opposite sense. From this behaviour it follows that over the more active hemisphere the corona is denser and hotter. Between density Ne and temperature T holds the relation: Ne = 10−10T3. The real asymmetry was strengthened by a phase difference of the two hemispheres. This phase shift is subject to a long period that contains 8 eleven-year cycles. The intensity of the individual cycles follows the same long period. With low maxima of solar activity the northern hemisphere precedes, with high maxima the southern hemisphere (Figure 3).

Keywords

Phase Shift Northern Hemisphere Solar Activity Phase Difference Southern Hemisphere 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1971

Authors and Affiliations

  • M. Waldmeier
    • 1
  1. 1.Swiss Federal ObservatoryZürichSwitzerland

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