On the statistics of maximum sunspot numbers

Details On the statistics of maximum sunspot numbers On the statistics of maximum sunspot numbers

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jastp..60.1707s&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 60, Issue 17, p. 1707-1710.

Physics

2

Scientific paper

On the basis of the statistics of extremes (i.e. Gumbels first asymptotic distribution)and the characteristics of cycles 9-22 (the most reliable sunspot cycles) the magnitude of the cyclepeaks is studied. The analysis is based on the quasi-periodic solar activity which has a main periodof approximately 22 years. According to this, we conclude that the odd and even cycles showdifferent behaviors. This statistical evidence can be considered a vehicle for the betterunderstanding of the physical processes related to the Sun. Thus, the results of this analysissupport previous findings that cycle 23 should be very active, causing important phenomena in theEarths environment.

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