中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes

文献类型:期刊论文

作者Yan, Y.1,2; Huang, J.1; Chen, B.1; Liu, Y.1; Tan, C.1
刊名ADVANCES IN SPACE RESEARCH
出版日期2010-08-16
卷号46期号:4页码:413-418
关键词Solar activities Solar flares Solar radio bursts Fine structures CME
英文摘要Radio bursts with fine structures in decimetric-centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1-2 GHz, 2.6-3.8 GHz, and 5.2-7.6 GHz at NAOC/Huairou with very high temporal (1.25-8 ms) and spectral (4-20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.
收录类别SCI
语种英语
WOS记录号WOS:000280940500007
源URL[http://ir.bao.ac.cn/handle/114a11/7715]  
专题国家天文台_太阳物理研究部
作者单位1.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
2.State Key Lab Space Weather, Beijing 100080, Peoples R China
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GB/T 7714
Yan, Y.,Huang, J.,Chen, B.,et al. Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes[J]. ADVANCES IN SPACE RESEARCH,2010,46(4):413-418.
APA Yan, Y.,Huang, J.,Chen, B.,Liu, Y.,&Tan, C..(2010).Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes.ADVANCES IN SPACE RESEARCH,46(4),413-418.
MLA Yan, Y.,et al."Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes".ADVANCES IN SPACE RESEARCH 46.4(2010):413-418.

入库方式: OAI收割

来源:国家天文台

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