Running waves in the sunspot chromosphere

被引:0
|
作者
D. Yu. Kolobov
N. I. Kobanov
机构
[1] Russian Academy of Sciences,Institute of Solar
来源
Geomagnetism and Aeronomy | 2009年 / 49卷
关键词
Solar Phys; Propagation Speed; Phase Speed; Chevron; Power Diagram;
D O I
暂无
中图分类号
学科分类号
摘要
Running waves at the chromospheric level (Hα) in sunspots are studied. Propagating 3-min oscillations are shown to be typical of many spots. Presumably, they propagate along the vertical magnetic-field lines. Their propagation speed is measured. According to our analysis, the 5-min oscillations propagating in the penumbral chromosphere are not a continuation of the 3-min umbral oscillations. The wavelength and propagation speed of the running penumbral waves are determined.
引用
收藏
页码:935 / 939
页数:4
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