Toroidal magnetic field of the Sun from data on Hale-rule-violating sunspot groups

被引：22

作者：

Khlystova, A. I. ^{[1
]}

Sokoloff, D. D. ^{[2
]}

机构：

[1] Russian Acad Sci, Siberian Div, Inst Solar Terr Phys, Irkutsk 664033, Russia

[2] Moscow MV Lomonosov State Univ, Dept Phys, Moscow 119991, Russia

来源：

ASTRONOMY REPORTS | 2009年 / 53卷 / 03期

基金：

美国国家科学基金会; 俄罗斯基础研究基金会; 中国国家自然科学基金; 美国国家航空航天局;

关键词：

HELICITY;

D O I：

10.1134/S106377290903010X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The latitude-time distribution of sunspot groups violating Hale polarity rule is considered for 1988-2004. This distribution exhibits a cyclic behavior similar to the general 11-year sunspot-activity cycle. The relative number of violating groups is used to estimate the ratio of the fluctuating and regular components of the toroidal magnetic field at the base of the convection zone.

引用

页码：281 / 285

页数：5

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