KMS of Xinjiang Astronomical Observatory, CAS
| Evolvement of microwave spike bursts in a solar flare on 2006 December 13 | |
Tang, Jian-Fei1,2,3 ; Wu, De-Jin2; Wan, Jun-Lin1,4; Chen, Ling2; Tan, Cheng-Ming3
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| 2021-08-01 | |
| Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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| ISSN | 1674-4527 |
| Volume | 21Issue:6Pages:148 |
| Contribution Rank | 1 |
| Abstract | Solar radio spikes are one of the most intriguing spectral types of radio bursts. Their very short lifetimes, small source size and super-high brightness temperature indicate that they should be involved in some strong energy release, particle acceleration and coherent emission processes closely related to solar flares. In particular, for the microwave spike bursts, their source regions are much close to the related flaring source region which may provide the fundamental information of the flaring process. In this work, we identify more than 600 millisecond microwave spikes which recorded by the Solar Broadband Radio Spectrometer in Huairou (SBRS/Huairou) during an X3.4 solar flare on 2006 December 13 and present a statistical analysis about their parametric evolution characteristic. We find that the spikes have nearly the same probability of positive and negative frequency drifting rates not only in the flare rising phase, but also in the peak and decay phases. So we suppose that the microwave spike bursts should be generated by shock-accelerated energetic electrons, just like the terminational shock (TS) wave produced by the reconnection outflows near the loop top. The spike bursts occurred around the peak phase have the highest central frequency and obviously weak emission intensity, which imply that their source region should have the lowest position with higher plasma density due to the weakened magnetic reconnection and the relaxation of TS during the peak phase. The right-handed polarization of the most spike bursts may be due to the TS lying on the top region of some very asymmetrical flare loops. |
| Keyword | Sun activity Sun flares Sun radio radiation |
| DOI | 10.1088/1674-4527/21/6/148 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | ELECTRON-CYCLOTRON MASER ; RADIO SPIKES ; FINE-STRUCTURE ; ACCELERATION ; RADIATION ; SPECTROMETER ; RECONNECTION ; INSTABILITY ; CALIBRATION ; PULSATIONS |
| Funding Project | National Natural Science Foundation of China[11673055] ; National Natural Science Foundation of China[41531071] ; National Natural Science Foundation of China[11873018] ; National Natural Science Foundation of China[11773061] ; National Natural Science Foundation of China[11790301] ; National Natural Science Foundation of China[11973057] ; Tianshan Youth fund[2017Q401] ; Key Laboratory of Solar Activity at National Astronomical Observatories, CAS ; [2018-XBQNXZ-A-009] ; [2017-XBQNXZ-A-007] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000684228500001 |
| Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
| Funding Organization | National Natural Science Foundation of China ; Tianshan Youth fund ; Key Laboratory of Solar Activity at National Astronomical Observatories, CAS |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/4222 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Tang, Jian-Fei |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Purple Mt Observ, Key Lab Planetary Sci, Nanjing 210023, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100101, Peoples R China 4.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Tang, Jian-Fei,Wu, De-Jin,Wan, Jun-Lin,et al. Evolvement of microwave spike bursts in a solar flare on 2006 December 13[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2021,21(6):148. |
| APA | Tang, Jian-Fei,Wu, De-Jin,Wan, Jun-Lin,Chen, Ling,&Tan, Cheng-Ming.(2021).Evolvement of microwave spike bursts in a solar flare on 2006 December 13.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,21(6),148. |
| MLA | Tang, Jian-Fei,et al."Evolvement of microwave spike bursts in a solar flare on 2006 December 13".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 21.6(2021):148. |
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| Tang-2021-Evolvement（412KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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