Gyrosynchrotron Process of a Rare Large Type-Ⅳμ Burst Associated with Coronal Mass Ejection

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作者：
Ji Shuchen Chen Xiaojuan Beijing Astronomical Observatory The Chinese Academy of Sciences Beijing China Yunnan Observatory The Chinese Academy of Sciences Kunming China National Astronomical Observatories The Chinese Academy [100080 ,650011 ]
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来源：
云南天文台台刊 | 1999年 / S1期
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P182.22 [];
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摘要：
A large Type Ⅳμ solar radio burst was observed at Yunnan observatory on December 16, 1988. The burst was associated by a coronal mass ejection (CME) with the radio signature of Type Ⅱ and Type Ⅳ bursts. On the basis of Beijing Huairou magnetogram of AR5278, power law distribution of electrons of the source region is calculated. It is suggested that the Type Ⅳμ burst associated with CME was due to the gyrosynchrotron radiation of high energy electrons trapped by magnetic field. Finally, some quantitative and qualitative explanations are proposed.
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页码：452 / 456
页数：5
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