Does the Babcock-Leighton mechanism operate on the Sun?

被引：56

作者：

Kitchatinov, L. L. ^{[1
,2
]}

Olemskoy, S. V. ^{[1
]}

机构：

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

[2] Russian Acad Sci, Pulkovo Astron Observ, St Petersburg 196140, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2011年 / 37卷 / 09期

基金：

俄罗斯基础研究基金会;

关键词：

Sun: magnetic fields; sunspots; dynamo; SOLAR DYNAMO MODEL; MAGNETIC-FIELD; CYCLE; ROTATION; WAVES;

D O I：

10.1134/S0320010811080031

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The contribution of the Babcock-Leighton mechanism to the generation of the Sun's poloidal magnetic field is estimated from sunspot data for three solar cycles. Comparison of the derived quantities with the A-index of the large-scale magnetic field suggests a positive answer to the question posed in the title of this paper.

引用

页码：656 / 658

页数：3

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