Axisymmetric sunspot oscillations

被引：0
|
作者：
Bogdan, TJ [1 ]
机构：
[1] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
来源：
HIGH RESOLUTION SOLAR PHYSICS: THEORY, OBSERVATIONS, AND TECHNIQUES | 1999年 / 183卷
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：
A discussion of some elementary considerations encountered in the study of the oscillations of axisymmetric sunspot; equilibria is presented. An expansion method is proposed for converting the relevant oscillation equations to a form that is better suited to numerical computation. In so doing, it is demonstrated that thin flux tube and flat canopy approximations are capable of providing physical insight onto the morphology of the oscillations in the deep submerged root of the sunspot and the far-flung outlying penumbral canopy.
引用
收藏
页码：78 / 86
页数：9
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