中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
MICROWAVE ZEBRA PATTERN STRUCTURES IN THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15

文献类型:期刊论文

作者Tan, Baolin1; Yan, Yihua1; Tan, Chengming1; Sych, Robert1,2; Gao, Guannan3
刊名ASTROPHYSICAL JOURNAL
出版日期2012-01-10
卷号744期号:2
关键词magnetic fields plasmas Sun: flares Sun: radio radiation
英文摘要A zebra pattern (ZP) structure is the most intriguing fine structure on the dynamic spectrograph of a solar microwave burst. On 2011 February 15, an X2.2 flare event erupted on the solar disk, which is the first X-class flare since the solar Schwabe cycle 24. It is interesting that there are several microwave ZPs observed by the Chinese Solar Broadband Radio Spectrometer (SBRS/Huairou) at a frequency of 6.40-7.00 GHz (ZP1) and at a frequency of 2.60-2.75 GHz (ZP2) and by the Yunnan Solar Broadband Radio Spectrometer (SBRS/Yunnan) at a frequency of 1.04-1.13 GHz (ZP3). The most important phenomenon is the unusual high-frequency ZP structure (ZP1, up to 7.00 GHz) that occurred in the early rising phase of the flare and the two ZP structures (ZP2, ZP3) with relatively low frequencies that occurred in the decay phase of the flare. By scrutinizing the current prevalent theoretical models of ZP structure generations and comparing their estimated magnetic field strengths in the corresponding source regions, we suggest that the double plasma resonance model is the most probable one for explaining the formation of microwave ZPs, which may derive the magnetic field strengths at about 230-345 G, 126-147 G, and 23-26 G in the source regions of ZP1, ZP2, and ZP3, respectively.
收录类别SCI
语种英语
WOS记录号WOS:000298666400086
源URL[http://ir.bao.ac.cn/handle/114a11/6180]  
专题国家天文台_太阳物理研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
2.Russian Acad Sci, Siberian Branch, Inst Solar Terr Phys, Irkutsk 664033, Russia
3.Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, Kunming 650011, Yunnan Province, Peoples R China
推荐引用方式
GB/T 7714
Tan, Baolin,Yan, Yihua,Tan, Chengming,et al. MICROWAVE ZEBRA PATTERN STRUCTURES IN THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15[J]. ASTROPHYSICAL JOURNAL,2012,744(2).
APA Tan, Baolin,Yan, Yihua,Tan, Chengming,Sych, Robert,&Gao, Guannan.(2012).MICROWAVE ZEBRA PATTERN STRUCTURES IN THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15.ASTROPHYSICAL JOURNAL,744(2).
MLA Tan, Baolin,et al."MICROWAVE ZEBRA PATTERN STRUCTURES IN THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15".ASTROPHYSICAL JOURNAL 744.2(2012).

入库方式: OAI收割

来源:国家天文台

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