Prediction of sunspot number amplitude and solar cycle length for cycles 24 and 25

被引:47
作者
Rigozo, N. R. [1 ]
Souza Echer, M. P. [2 ]
Evangelista, H. [3 ]
Nordemann, D. J. R. [2 ]
Echer, E. [2 ]
机构
[1] INPE CRS, Ctr Reg Sul Pesquisas Especiais, BR-97105970 Santa Maria, RS, Brazil
[2] Inst Nacl Pesquisas Espaciais, BR-12245970 Sao Jose Dos Campos, SP, Brazil
[3] Univ Estado Rio de Janeiro, Lab Radioecol & Mudancas Globais, Dept Biofis & Biometria, BR-20550013 Rio De Janeiro, Brazil
关键词
Prediction solar activity; Sunspot number time series; Spectral analysis; Multiresolution analysis; SPECTRAL CHARACTERISTICS; MAXIMUM; MINIMUM; INDEXES; SERIES; SIZE; FLUX; SUN;
D O I
10.1016/j.jastp.2010.09.005
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The prediction of solar activity strength for solar cycles 24 and 25 is made on the basis of extrapolation of sunspot number spectral components. Monthly sunspot number data during the 1850-2007 interval (solar cycles 9-23) are decomposed into several levels and searched for periodicities by iterative regression in each level. For solar cycle 24, the peak is predicted in November 2013 with a sunspot number of 113.3. The cycle is expected to be weak, with a length of 133 mo (months) or 11.1 yr. The sunspot number maximum in cycle 25 is predicted to occur in April 2023 with a sunspot number 132.1 and a solar cycle length of 118 mo or 9.8 yr. Thus, solar cycle 24 is predicted to have an intensity 23% lower than cycle 23, and cycle 25 will be 5% lower than cycle 23. (C) 2010 Elsevier Ltd. All rights reserved.
引用
收藏
页码:1294 / 1299
页数:6
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