Some notes concerning the prediction of the amplitude of the two solar activity cycles
| dc.creator | Tlatov, A. G. | |
| dc.date | 2007-06-12 | |
| dc.date.accessioned | 2026-07-07T08:05:13Z | |
| dc.date.available | 2026-07-07T08:05:13Z | |
| dc.description | 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). | |
| dc.description | 5 pages, 5 figures | |
| dc.identifier | https://arxiv.org/abs/0706.1624 | |
| dc.identifier | http://arxiv.org/abs/0706.1624 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/130213 | |
| dc.subject | Astrophysics | |
| dc.title | Some notes concerning the prediction of the amplitude of the two solar activity cycles | |
| dc.type | text |