Radioheliograph Observations of Microwave Bursts with Zebra Structures
文献类型:期刊论文
作者 | Altyntsev, A. T.1; Lesovoi, S. V.1; Meshalkina, N. S.1; Sych, R. A.1,2; Yan, Y.2![]() |
刊名 | SOLAR PHYSICS
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出版日期 | 2011-10-01 |
卷号 | 273期号:1页码:163-177 |
关键词 | Dynamic spectrum Microwave emission Radio bursts Solar flares Zebra pattern |
英文摘要 | The so-called zebra structures in radio dynamic spectra, specifically their frequencies and frequency drifts of emission stripes, contain information on the plasma parameters in the coronal part of flare loops. This paper presents observations of zebra structures in a microwave range. Dynamic spectra were recorded by Chinese spectro-polarimeters in the frequency band close to the working frequencies of the Siberian Solar Radio Telescope. The emission sources are localized in the flare regions, and we are able to estimate the plasma parameters in the generation sites using X-ray data. The interpretation of the zebra structures in terms of existing theories is discussed. The conclusion has been arrived at that the preferred generation mechanism of zebra structures in the microwave range is the conversion of plasma waves to electromagnetic emission on the double plasma resonance surfaces distributed across a flare loop. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000297125700011 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7894] ![]() |
专题 | 国家天文台_太阳物理研究部 |
作者单位 | 1.Inst Solar Terr Phys SB RAS, Irkutsk 664033, Russia 2.CAS, Key Lab Solar Activ, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Altyntsev, A. T.,Lesovoi, S. V.,Meshalkina, N. S.,et al. Radioheliograph Observations of Microwave Bursts with Zebra Structures[J]. SOLAR PHYSICS,2011,273(1):163-177. |
APA | Altyntsev, A. T.,Lesovoi, S. V.,Meshalkina, N. S.,Sych, R. A.,&Yan, Y..(2011).Radioheliograph Observations of Microwave Bursts with Zebra Structures.SOLAR PHYSICS,273(1),163-177. |
MLA | Altyntsev, A. T.,et al."Radioheliograph Observations of Microwave Bursts with Zebra Structures".SOLAR PHYSICS 273.1(2011):163-177. |
入库方式: OAI收割
来源:国家天文台
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