Quasibiennial oscillations of the north-south asymmetry

被引:23
|
作者
Badalyan, OG [1 ]
Obridko, VN
Rybák, J
Sykora, J
机构
[1] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radiowave Radiow, Troitsk 412190, Russia
[2] Slovak Acad Sci, Astron Inst, Tatranska Lomnica 05960, Slovakia
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1134/1.2010655
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The north-south (N-S) asymmetry of the solar activity (A), which reflects differences in the behavior of the northern and southern hemispheres of the Sun, is studied using data on the brightness of the coronal green line, the total number and area of sunspots, and the net magnetic flux. The spatial and temporal distributions and correlations between the A values represented by these indices are considered. The characteristic time variations in A are similar for all the indices, on both long and short time scales. Quasibiennial oscillations (QBOs) can be traced in the asymmetries of all four indices. A detailed study of the QBOs is carried out based on spectral-variation and wavelet analyses. Long-term increases and decreases occur synchronously in the asymmetries of various indices and are Much more pronouriced in A than in the indices themselves. A negative correlation between the power of the QBOs and the asymmetry of A can be traced; it is most clearly manifest as a substantial diminishing of the QBOs during the mid-1960s, which coincided with an especially strong increase in A. Our analysis shows that the N-S asymmetry is probably a fundamental property that Controls the coupling and degree of coincidence between the magnetic-field-generation mechanisms operatirig in the northern and Southern hemispheres. (c) 2005 Pleiades Publishing, Inc.
引用
收藏
页码:659 / 670
页数:12
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