The predicted size of cycle 23 based on the inferred three-cycle quasi-periodicity of the planetary index Ap

被引:58
作者
Ahluwalia, HS [1 ]
机构
[1] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1998年 / 103卷 / A6期
关键词
D O I
10.1029/98JA00960
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A review of the solar and the geophysical data for the last 6 decades indicates the existence of a three-solar-activity-cycle quasi-periodicity in them. It is also present in other data sets extending over several centuries. A new cycle may have started after 1996. If true, cycle 23 will be more modest (a la cycle 17) with an annual mean sunspot number count of 119.3 +/- 30 at the maximum. This inference is in contrast to the predictions of some of the solar astronomers who are predicting a very active cycle 23 (a la cycle 19).
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页码:12103 / 12109
页数:7
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