A nonlinear mathematical model for the solar cyclicity and prospects for reconstructing the solar activity in the past

Details A nonlinear mathematical model for the solar cyclicity and prospects for reconstructing the solar activity in the past A nonlinear mathematical model for the solar cyclicity and prospects for reconstructing the solar activity in the past

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997astl...23..742n&link_type=abstract

Astronomy Letters, Volume 23, Issue 6, November 1997, pp.742-748; Pis'ma v Astronomicheskii Zhurnal, Vol. 23, p. 851

Astronomy and Astrophysics

Astronomy

34

Scientific paper

Based on Krylov-Bogolyubov's approach to the description of weakly nonlinear oscillatory processes, we analyze the nonstationary frequency-amplitude structure of the solar activity on large time scales. Using the nonlinear description and Schove's data on the epochs of extrema of 11-year solar cycles in the past, we reconstruct the yearly average Wolf numbers in 1100-1700. We discuss the agreement between the derived series and circumstantial evidence and the satisfaction of Gnevyshev-Ohl's rule in the past 900 years.

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