中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
On the wave mode of subsecond pulses in the cm-range

文献类型:期刊论文

作者Meshalkina, NS; Altyntsev, AT; Sych, RA; Chernov, GP; Yan, YH
刊名SOLAR PHYSICS
出版日期2004-05-01
卷号221期号:1页码:85-99
英文摘要In this paper we determined the wave mode of subsecond pulses (SSP). We used data on pulses with a degree of polarization over 30%, with the sources located at -60 to +60 deg from the central meridian, for the period 2000-2002. The superposition of SSRT radio maps and MDI magnetograms has shown that radio SSP sources are typically located near the polarity inversion line of the active region magnetic field. Such an arrangement indicates that SSP sources are located at the tops of magnetic loops. The ordinary mode of electromagnetic radiation is recorded in SSP sources located from the inversion line by no less than about 10 arc sec.
收录类别SCI
语种英语
WOS记录号WOS:000222347600008
源URL[http://ir.bao.ac.cn/handle/114a11/6950]  
专题国家天文台_太阳物理研究部
作者单位1.Inst Solar Terr Phys, Irkutsk, Russia
2.Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radio Wave Propa, Troitsk 142092, Russia
3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Meshalkina, NS,Altyntsev, AT,Sych, RA,et al. On the wave mode of subsecond pulses in the cm-range[J]. SOLAR PHYSICS,2004,221(1):85-99.
APA Meshalkina, NS,Altyntsev, AT,Sych, RA,Chernov, GP,&Yan, YH.(2004).On the wave mode of subsecond pulses in the cm-range.SOLAR PHYSICS,221(1),85-99.
MLA Meshalkina, NS,et al."On the wave mode of subsecond pulses in the cm-range".SOLAR PHYSICS 221.1(2004):85-99.

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来源:国家天文台

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