AN OBSERVATIONAL EXAMINATION OF MODELS FOR SUNSPOT MAGNETIC-FIELD CONFIGURATIONS

被引：21

作者：

ADAM, MG

机构：

[1] Department of Astrophysics, Oxford

来源：

SOLAR PHYSICS | 1990年 / 125卷 / 01期

关键词：

D O I：

10.1007/BF00154777

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The magnetic field configuration for an isolated, nearly circular sunspot has been obtained from measurements at some 100 points in the spot. The observations are compared with theoretical models for the field configuration of an isolated, axially-symmetric sunspot. The results support the Schlüter, Temesváry model with no return flux and a limiting field line inclination of ~70°. © 1990 Kluwer Academic Publishers.

引用

页码：37 / 44

页数：8

共 14 条

[1]

ADAM MG, 1985, SOL PHYS, V96, P27, DOI 10.1007/BF00239792

[2] ROLE OF MAGNETIC FORCES IN SUNSPOT EQUILIBRIUM [J].