LARGE-SCALE INTERNAL MAGNETIC-FIELD OF THE SUN

被引：0
|
作者：
DUDOROV, AE
KRIVODUBSKIJ, VN
RUZMAIKIN, AA
RUZMAIKINA, TV
机构：
[1] KIEV SHEVCHENKO UNIV, ASTRON OBSERV, KIEV 252053, UKRAINE, USSR
[2] IZMIRAN, TROITSK 142092, USSR
[3] INST PHYS EARTH, MOSCOW 123810, USSR
来源：
IAU SYMPOSIA | 1990年 / 138期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The behaviour of the magnetic field during the formation and evolution of the Sun is investigated. It is shown that an internal poloidal magnetic field of the order of 10(4) - 10(5) G near the core of the Sun may be compatible with differential rotation and with torsional waves, travelling along the magnetic field lines (Dudorov et al., 1989).
引用
收藏
页码：391 / 394
页数：4
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