Prediction of solar activity on the basis of spectral characteristics of sunspot number

被引:29
作者
Echer, E
Rigozo, NR
Nordemann, DJR
Vieira, LEA
机构
[1] Inst Nacl Pesquisas Espaciais, BR-12201970 Sao Jose Dos Campos, Brazil
[2] Fac Tecnol Thereza Porto Marques, BR-12308320 Jacerei, Brazil
关键词
solar physics; astrophysics and astronomy (instruments and techniques; general or miscellaneous; photosphere and chromosphere);
D O I
10.5194/angeo-22-2239-2004
中图分类号
P1 [天文学];
学科分类号
0704 [天文学];
摘要
Prediction of solar activity strength for solar cycles 23 and 24 is performed on the basis of extrapolation of sunspot number spectral components. Sunspot number data during 1933-1996 periods (solar cycles 17-22) are searched for periodicities by iterative regression. The periods significant at the 95% confidence level were used in a sum of sine series to reconstruct sunspot series, to predict the strength of solar cycles 23 and 24. The maximum peak of solar cycles is adequately predicted (cycle 21: 158+/-13.2 against an observed peak of 155.4; cycle 22: 178+/-13.2 against 157.6 observed). Solar cycle 23 was predicted to have a peak in 2000 with maximum amplitude of 125+/-13.2, in good agreement with the 119.6 observed. The minimum of solar cycle 23 is predicted to occur around 2007-2008. For solar cycle 24, the maximum is predicted to occur in 2012 (115+/-13.2) or 2013 (117+/-13.2) and this shall be a very weak solar cycle.
引用
收藏
页码:2239 / 2243
页数:5
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