Dynamics of the quiet solar chromosphere

被引：0
|
作者：
Rutten, RJ [1 ]
Lites, BW [1 ]
Berger, TE [1 ]
Shine, RA [1 ]
机构：
[1] Sterrekundig Inst, NL-3508 TA Utrecht, Netherlands
来源：
SOLAR AND STELLAR ACTIVITY: SIMILARITIES AND DIFFERENCES | 1999年 / 158卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The solar chromosphere has never been static although it was often modeled so. Even the quiet-sun internetwork chromosphere has become thoroughly dynamic with the acoustic shock interpretation of the Ca II K-2V grains. We concentrate on the latter in this brief review. Recent analysis of Advanced Stokes Polarimeter (ASP) data confirms that their excitation is more likely set acoustically than magnetically. TRACE imagery permits seeing-free studies of their occurrence patterns.
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页码：249 / 259
页数：11
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