Specific features of long-period oscillations of sunspots and photosphere according to the MDI (SOHO) data

被引:0
|
作者
V. I. Efremov
L. D. Parfinenko
A. A. Solov’ev
机构
[1] Russian Academy of Sciences,Central (Pulkovo) Astronomical Observatory
来源
Geomagnetism and Aeronomy | 2013年 / 53卷
关键词
Period Oscillation; Wavelet Spectrum; Side Panel; Intensity Record; Sight Velocity;
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摘要
Long-period oscillations of the magnetic field and the line-of-sight velocity have been detected in sunspots based on the synchronous 90-h time series of magnetograms and dopplergrams obtained with the MDI(SOHO) device. The sunspot eigenmode (12–30 h), the periods of which nonlinearly depend on the magnetic field strength, predominates in the magnetic field oscillation spectrum. The mode, which is probably induced by motions of supergranulation cells (33 h), predominates in the sunspot line-of-sight velocity oscillation spectrum. A strong mode (33 h), which indicates that long-period quasi-oscillations of supergranulation exist, was also detected in the velocity power spectrum for a quiet photosphere, together with the known 5-min mode.
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页码:1016 / 1020
页数:4
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