Large-Scale Structure of the Sunspot Activity and the Background Magnetic Field Formation

被引：0
|
作者：
D.V. Erofeev
机构：
[1] Ussuriysk Observatory,
来源：
Solar Physics | 1999年 / 186卷
关键词：
Magnetic Field; Magnetic Flux; Solar Cycle; Modal Structure; Rotation Period;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Large-scale distribution of the sunspot activity of the Sun has been analyzed by using a technique worked out previously (Erofeev, 1997) to study long-lived, non-axisymmetric magnetic structures with different periods of rotation. Results of the analysis have been compared with those obtained by analyzing both the solar large-scale magnetic field and large-scale magnetic field simulated by means of the well-known flux transport equation using the sunspot groups as a sole source of new magnetic flux in the photosphere. A 21-year period (1964–1985) has been examined.
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页码：431 / 447
页数：16
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