Heating of solar filamentary magnetic flux tubes

被引：0
作者：
Dwivedi, R [1 ]
Singh, RN
机构：
[1] Banaras Hindu Univ, Inst Technol, Dept Appl Phys, Varanasi 221005, Uttar Pradesh, India
[2] CSJM Univ, Dept Phys, Kanpur 208016, Uttar Pradesh, India
来源：
CURRENT SCIENCE | 2001年 / 80卷 / 01期
关键词：
D O I：
暂无
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
The sunspot regions are well-known sources of energetic charged particle emissions and numerous wave mode generations. It is shown that the high frequency electromagnetic waves generated by synchrotron process, at times, could be cross-modulated by low frequency p-mode oscillations. The analyses of recorded electromagnetic field strength and seismic waves would depict interesting features of the originating sunspot regions.
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页码：64 / 67
页数：4
相关论文
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