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![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL
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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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