NONTHERMAL RADIO-EMISSION ASSOCIATED WITH A CORONAL DISCONNECTION EVENT

被引：4

作者：

GOPALSWAMY, N ^{[1
]}

KUNDU, MR ^{[1
]}

STCYR, OC ^{[1
]}

机构：

[1] NASA,GODDARD SPACE FLIGHT CTR,ALLIEDSIGNAL TECHN SERV CORP,GREENBELT,MD 20771

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 424卷 / 02期

关键词：

SOLAR-TERRESTRIAL RELATIONS; SUN; ACTIVITY; CORONA; FLARES; RADIO RADIATION;

D O I：

10.1086/187293

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have found possible radio signatures of a coronal disconnection event observed by the Solar Maximum Mission Coronagraph/Polarimeter. The radio emission seems to be produced by charged particles accelerated during the same reconnection process which is responsible for the disconnection event. We discuss the implications of the radio emission characteristics to the reconnection process.

引用

页码：L135 / L138

页数：4

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