Relationship of Asymmetries in the Distribution of Solar Tracer Activity and Generation of the Solar Magnetic Field

被引：0
|
作者：
Sokolov, D. D. [1 ,2 ]
Yushkov, E. V. [1 ,3 ]
机构：
[1] Moscow State Univ, Moscow 119991, Russia
[2] Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere & Radio Wav, Troitsk 108840, Moscow, Russia
[3] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2024年 / 64卷 / 07期
关键词：
sunspots; Maunder Minimum; solar dynamo; MAUNDER MINIMUM;
D O I：
10.1134/S0016793224700245
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 cause of the asymmetry in the sunspot distribution in the northern and southern hemispheres of the Sun at the end of the Maunder Minimum is studied. It is demonstrated that the expected asymmetry of generation sources is insufficient for such an explanation. To study the influence of asymmetry of generation sources, numerical simulation is used, based on modifications to the Parker model.
引用
收藏
页码：1163 / 1166
页数：4
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