Simulations of Waves in Sunspots

被引：0
|
作者：
Khomenko, E. [1 ]
机构：
[1] Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Tenerife, Spain
来源：
SOLAR-STELLAR DYNAMOS AS REVEALED BY HELIO AND ASTEROSEISMOLOGY: GONG 2008/SOHO 21 | 2009年 / 416卷
关键词：
MAGNETIZED SOLAR ATMOSPHERE; RUNNING PENUMBRAL WAVES; P-MODE ABSORPTION; ACTIVE REGIONS; MAGNETOACOUSTIC WAVES; UMBRAL OSCILLATIONS; TRANSITION REGION; STRATIFIED ATMOSPHERE; OPTICAL TELESCOPE; INVERSION METHODS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A magnetic field modifies the properties of waves in a complex way. Significant advances have been made recently in our understanding of the physics of waves in solar active regions with the help of analytical theories, numerical simulations, and high-resolution observations. In this contribution we review the current ideas in the field, with the emphasis on theoretical models of waves in sunspots.
引用
收藏
页码：31 / 40
页数：10
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