Asymmetries during the maximum phase of solar cycle 22

Details Asymmetries during the maximum phase of solar cycle 22 Asymmetries during the maximum phase of solar cycle 22

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..157..315j&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 157, no. 1-2, p. 315-324

Physics

21

Asymmetry, Solar Activity, Solar Cycles, Sun, Events, Occurrences, Solar Physics

Scientific paper

This paper presents the results of studies of the asymmetries (N-S and E-W) for different manifestations of solar activity events (sunspot groups, H alpha flares and active prominences/ filaments) during the maximum-phase (1989-1991) of solar cycle 22. During the period considered, the results obtained show the existence of a real N-S asymmetry, whereas the E-W asymmetry may exist only for H alpha flares. There is no definite relationship between the asymmetries and the occurrence of events; however, around low activity sometimes we find enhanced symmetry, and low asymmetry around high activity. Our study suggests a good agreement with similar studies made by others.

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