SPIKE EMISSION AT 21 CM WAVELENGTH IN POST-FLARE LOOPS | |
FU, QJ1; LI, CS2; Gong YF(龚元芳)3; LI, W1; ZHAO, B1; SHANG, QZ3; Lv SQ(吕松泉)3; Hu HM(胡汉明)3 | |
发表期刊 | SOLAR PHYSICS
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1993-02-01 | |
卷号 | 143期号:2页码:317-326 |
DOI | 10.1007/BF00646490 |
产权排序 | 第3完成单位 |
收录类别 | SCI |
摘要 | Electron-cyclotron maser instability produced by accelerated energetic electrons is today's most favoured process for spike emission on ultra-short time scales at dm wavelengths. The process of electron acceleration occurs primarily in pre-impulsive and impulsive phases. We present observations of spike bursts at 21 cm in a limb event that occurred in AR 5629 on 1989 August 17. Optical observations of the event from Beijing Astronomical Observatory show coronal loops that interact just before the spike groups appeared. This implies that additional particle acceleration might be produced by the interaction between emerging loops and original large loops, and become the source of the energetic electrons responsible for the spike emission appearing in the descending phase. Some important parameters are deduced. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0038-0938 |
URL | 查看原文 |
WOS记录号 | WOS:A1993KL43600009 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | MILLISECOND ; BURSTS ; GHZ |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4067 |
专题 | 其他 |
通讯作者 | FU, QJ |
作者单位 | 1.Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China (BAO) 2.Department of Astronomy, Naujing University, Nanjing 210008, China (NJU) 3.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China (YAO) |
推荐引用方式 GB/T 7714 | FU, QJ,LI, CS,Gong YF,et al. SPIKE EMISSION AT 21 CM WAVELENGTH IN POST-FLARE LOOPS[J]. SOLAR PHYSICS,1993,143(2):317-326. |
APA | FU, QJ.,LI, CS.,Gong YF.,LI, W.,ZHAO, B.,...&Hu HM.(1993).SPIKE EMISSION AT 21 CM WAVELENGTH IN POST-FLARE LOOPS.SOLAR PHYSICS,143(2),317-326. |
MLA | FU, QJ,et al."SPIKE EMISSION AT 21 CM WAVELENGTH IN POST-FLARE LOOPS".SOLAR PHYSICS 143.2(1993):317-326. |
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Spike emission at 21(653KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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