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![]() ![]() ![]() |
刊名 | ADVANCES IN SPACE RESEARCH
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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 |
推荐引用方式 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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