Quasi-periodic reversals of radio polarization at 17 GHz observed in the 2002 April 21 solar event | |
Huang, GL1; Lin J(林隽)2,3 | |
刊名 | ASTROPHYSICAL JOURNAL |
2006-03-10 | |
卷号 | 639期号:2页码:L99-L102 |
关键词 | polarization Sun : activity Sun : radio radiation |
ISSN号 | 0004-637X |
通讯作者 | Huang, GL (reprint author), Chinese Acad Sci, Purple Mt Observ, 2 W Beijing Rd, Nanjing 210008, Peoples R China. |
产权排序 | 第二完成单位 |
英文摘要 | We investigate high spatial resolution radio polarization data obtained by the Nobeyama Radioheliograph (NoRH) and high time resolution data observed with the Nobeyama Radio Polarimeters (NoRP) during the well-studied flare/CME event of 2002 April 21. A 17 GHz radio source at the loop top was seen by NoRH to move upward together with the expanding flare loops at a speed of around 10 km s(-1). In the 5 minutes before the source began its upward motion, the Stokes V of the radio signals at 17 GHz showed quasi-periodic reversals between left-circular polarization (LCP) and right-circular polarization (RCP). Following this interval, the polarizations gradually turned to LCP. During this period, the polarization of the corresponding footpoint source maintained the RCP sense. The reversal of Stokes V between RCP and LCP was also detected at lower frequencies (1-2 GHz) by NoRP, without spatial resolution. The observed reversals between RCP and LCP of the radio signals from the top of the flare loop system can be taken as evidence that magnetic energy is released or energetic particles are produced at the magnetic reconnection site in a quasi-periodic fashion. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | CORONAL MASS EJECTION ; NOBEYAMA RADIOHELIOGRAPH ; MAGNETIC-FIELD ; X1.5 FLARE ; RHESSI ; RECONNECTION ; MICROWAVE ; BURSTS ; EMISSION ; TRACE |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/1538-4357/639/2/L99/ |
语种 | 英语 |
WOS记录号 | WOS:000235837200014 |
公开日期 | 2016-05-03 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6093] |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | 1.Purple Mountain Observatory, Chinese Academy of Sciences, 2 West Beijing Road, 210008 Nanjing, China 2.Yunnan Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, China 3.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 |
推荐引用方式 GB/T 7714 | Huang, GL,Lin J. Quasi-periodic reversals of radio polarization at 17 GHz observed in the 2002 April 21 solar event[J]. ASTROPHYSICAL JOURNAL,2006,639(2):L99-L102. |
APA | Huang, GL,&Lin J.(2006).Quasi-periodic reversals of radio polarization at 17 GHz observed in the 2002 April 21 solar event.ASTROPHYSICAL JOURNAL,639(2),L99-L102. |
MLA | Huang, GL,et al."Quasi-periodic reversals of radio polarization at 17 GHz observed in the 2002 April 21 solar event".ASTROPHYSICAL JOURNAL 639.2(2006):L99-L102. |
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