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arXiv:0706.1624 (astro-ph)
[Submitted on 12 Jun 2007]

Title:Some notes concerning the prediction of the amplitude of the two solar activity cycles

Authors:A. G. Tlatov
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Abstract: The parameter G, which is determined from the general number of sunspots groups Ng according to the daily observations G=Sum(1/Ng)^2, is offered. This parameter is calculated for the days when there is at least one sunspots group. It characterizes the minimum epoch solar activity. Parameter G mounts to the maximum during the epoch close to the minimal activity of sunspots. According too the data of the sequence of sunspots group in Greenwich-USAF/NOAA observatory format, observation data of Kislovodsk solar station and also daily Wolf number the changes of parameter G during 100 years were reconstructed. It is demonstrated in the paper that parameter G's amplitude in minimal solar activity n is linked with the sunspot cycle's amplitude Wn+1. The 24th activity cycle prediction is calculated, which makes W24=135(+/-12).
Comments: 5 pages, 5 figures
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0706.1624 [astro-ph]
  (or arXiv:0706.1624v1 [astro-ph] for this version)
  https://doi.org/10.48550/arXiv.0706.1624

Submission history

From: Andrey Tlatov [view email]
[v1] Tue, 12 Jun 2007 08:09:49 UTC (160 KB)
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