Small-Amplitude Oscillations in Solar Filaments

被引：2
|
作者：
Mashnich, G. P. [1 ]
Bashkirtsev, V. S. [1 ]
Khlystova, A. I. [1 ]
机构：
[1] Russian Acad Sci, Insr Solar Terr Phys, Siberian Branch, Irkutsk 664033, Russia
来源：
ASTRONOMY REPORTS | 2012年 / 56卷 / 03期
基金：
俄罗斯基础研究基金会;
关键词：
QUIESCENT PROMINENCE; DOPPLER OSCILLATIONS; WAVELET ANALYSIS; HINODE/SOT; THREADS;
D O I：
10.1134/S1063772912030055
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The temporal and spatial properties of small-amplitude oscillations have been studied using spectral observations of motions in solar filaments carried out at the Sayan Solar Observatory (Institute of Solar-Terrestrial Physics, Russian Academy of Sciences). Oscillations with different periods and spatial scales exist simultaneously in filaments. Swaying motions of filaments in the plane of the sky have been detected. The character of these oscillatory motions is compared with oscillations in the Doppler velocity at the same filament sites.
引用
收藏
页码：241 / 249
页数：9
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