Development of solar flares and features of the fine structure of solar radio emission
- 作者: Chernov G.P.1,2, Fomichev V.V.2, Yan Y.1, Tan B.1, Tan C.1, Fu Q.1
- 
							隶属关系: 
							- Huairou Solar Observing Station
- Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
 
- 期: 卷 57, 编号 6 (2017)
- 页面: 738-751
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156451
- DOI: https://doi.org/10.1134/S0016793217060032
- ID: 156451
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详细
The reason for the occurrence of different elements of the fine structure of solar radio bursts in the decimeter and centimeter wavelength ranges has been determined based on all available data from terrestrial and satellite observations. In some phenomena, fast pulsations, a zebra structre, fiber bursts, and spikes have been observed almost simultaneously. Two phenomena have been selected to show that the pulsations of radio emission are caused by particles accelerated in the magnetic reconnection region and that the zebra structure is excited in a source, such as a magnetic trap for fast particles. The complex combination of unusual fiber bursts, zebra structure, and spikes in the phenomenon on December 1, 2004, is associated with a single source, a magnetic island formed after a coronal mass ejection.
作者简介
G. Chernov
Huairou Solar Observing Station; Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
							编辑信件的主要联系方式.
							Email: gchernov@izmiran.ru
				                					                																			                												                	中国, 							Beijing; Moscow						
V. Fomichev
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
														Email: gchernov@izmiran.ru
				                					                																			                												                	俄罗斯联邦, 							Moscow						
Y. Yan
Huairou Solar Observing Station
														Email: gchernov@izmiran.ru
				                					                																			                												                	中国, 							Beijing						
B. Tan
Huairou Solar Observing Station
														Email: gchernov@izmiran.ru
				                					                																			                												                	中国, 							Beijing						
Ch. Tan
Huairou Solar Observing Station
														Email: gchernov@izmiran.ru
				                					                																			                												                	中国, 							Beijing						
Q. Fu
Huairou Solar Observing Station
														Email: gchernov@izmiran.ru
				                					                																			                												                	中国, 							Beijing						
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