Gnevyshev Peaks in the CME Average Speeds in Cycle 23

Details Gnevyshev Peaks in the CME Average Speeds in Cycle 23 Gnevyshev Peaks in the CME Average Speeds in Cycle 23

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010soph..261..209k&link_type=abstract

Solar Physics, Volume 261, Issue 1, pp.209-213

Physics

1

Gnevyshev Peaks, Coronal Mass Ejections, Cycle 23

Scientific paper

Sunspots have a major 11-year cycle, but the three to four years near the maximum may show two or more peaks called Gnevyshev peaks. Earlier, it was reported that in Solar Cycle 23, the double peak in sunspot numbers was reflected in the electromagnetic radiations and coronal mass ejection (CME) frequencies in the solar atmosphere, but with phase differences. In this article, it is shown that the average CME speeds also show Gnevyshev peaks but with phase differences.

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