| 一个复杂太阳射电爆发及其微波源区特征的初步研究 |
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| 引用本文： | 汪敏,王昆山,谢瑞祥,施硕彪,王霖,刘玉英,李维华.一个复杂太阳射电爆发及其微波源区特征的初步研究[J].天文研究与技术,2004,1(1):56-63. |
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| 作者姓名： | 汪敏 王昆山 谢瑞祥 施硕彪 王霖 刘玉英 李维华 |
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| 作者单位： | [1]中国科学院国家天文台云南天文台,云南昆明650011 [2]云南省计算中心,云南昆明650023 [3]中国科学院国家天文台,北京100012 |
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| 基金项目： | 937资助项目(G2000078403). |
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| 摘 要： | 我国“太阳射电宽带频谱仪(0．7～7．6GHz)”于2001年10月19日观测到的复杂太阳射电大爆发，呈现许多有趣的特征。本文结合NoRH的高空分辨率成像观测资料，分析了该爆发的微波射电源区的演化特征及与射电辐射特征的关系。还发现微波源的缓慢运动，这可能与爆发所伴随的CME的形成有关。
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| 关 键 词： | 太阳 射电爆发 射电辐射 微波源 CME |
| 文章编号： | 1673-7673(2004)01-0056-08 |
| 修稿时间： | 2003年4月30日 |
Primary Research on a Complex Solar Radio Burst and its Characteristics of Microwave Sources |
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| WANG Min,WANG Kun-shan,XIE Rui-xiang,SHI Shuo-biao,WANG Lin,LIU Yu-ying,LI Wei-hua.Primary Research on a Complex Solar Radio Burst and its Characteristics of Microwave Sources[J].Astronomical Research & Technology,2004,1(1):56-63. |
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| Authors: | WANG Min WANG Kun-shan XIE Rui-xiang SHI Shuo-biao WANG Lin LIU Yu-ying LI Wei-hua |
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| Institution: | WANG Min~1,WANG Kun-shan~2,XIE Rui-xiang~1,SHI Shuo-biao~1,WANG Lin~1,LIU Yu-ying~3,LI Wei-hua~1 |
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| Abstract: | A very complex outstanding solar radio burst was observed with the wide-band spectrometer of NAOC on October 19,2001.This burst was characterized by a broader band (decameter to dcetimeter) burst followed by an more intense narrow-band burst at the lower frequencies (decimetric).NoRH (Nobeyama Radio Heliograph) observations about this event at 17 and 34 GHz showed that the cofiguration of radio sources included three sources,i.e.,a pre-existing source,a main source,and a disturbing source.The emission time profiles of these three sources were essentially different.The pre-existing source should be the manifestation of the heating process of the flare,and should be related to the complex component of the radio burst.The main source should be related to the continua of the radio burst.The disturbing source should be the trigger of this burst.Combining the data of NoRH,the evolution of microwave sources,as well as the relation between the sources evolution and the global features of the radio emissions are studied.Combining the data of MDI (Michelson Doppler Imager),we conclude that the pre-existing source should be near the feet of the coronal loop and the main source shoule be near the top of the loop or at least near the loop leg.Furthermore,the very slow moving of the main source has been found,it may be related to the formation of CME associated with this event. |
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| Keywords: | sun radio burst microwave source |
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