Ultra Low-Frequency Oscillations of a Solar Filament Observed by the GONG Network

被引:12
作者
Efremov, V. I. [1 ]
Parfinenko, L. D. [1 ]
Solov'ev, A. A. [1 ,2 ]
机构
[1] RAS, Cent Pulkovo Astron Observ, St Petersburg, Russia
[2] Kalmyk State Univ, Elista, Russia
关键词
Sun; Filament; Oscillations; Intensity; Magnetic field; LONG-PERIOD OSCILLATIONS; SUNSPOTS; MOTION; SOHO/MDI; WAVE;
D O I
10.1007/s11207-016-1021-z
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The data of ground-based telescopes of the Global Oscillation Network Group (GONG) obtained in the Ha line provide an opportunity to study the long-period oscillations of chromospheric filaments (quiescent prominences). For the first time, on the basis of time series of 5 days duration that we combined from the observations of three observatories of the GONG network, a new ultra-low mode with a period of between 20 and 30 hours was reliably detected in oscillations of a long-lived dark filament on the solar disk.
引用
收藏
页码:3357 / 3367
页数:11
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