Long-term oscillations in solar active regions based on magnetic fields and radio emission

被引：4
|
作者：
Nagovitsyn, Yu. A. [1 ]
Nagovitsyna, E. Yu. [1 ]
Abramov-Maximov, V. E. [1 ]
机构：
[1] Russian Acad Sci, Cent Astron Observ, St Petersburg 196140, Russia
来源：
ASTRONOMY REPORTS | 2013年 / 57卷 / 08期
关键词：
PERIOD OSCILLATIONS; SUNSPOT;
D O I：
10.1134/S1063772913080052
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A comparative analysis of sunspot oscillations and related radio sources in the active regions AR 8949, AR 8951, and AR 8953 is carried out using SOHO MDI data and simultaneous observations with the Nobeyama Radioheliograph, with a one-minute time resolution on scales of tens to hundreds of minutes. The radio sources in the selected active regions are similar to 40 000-60 000 km away from the corresponding spots, with the periods of long-term oscillations of the radio sources being similar to 12% longer.
引用
收藏
页码：636 / 640
页数：5
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