EVAPORATION CAUSES FLARE-RELATED RADIO-BURST CONTINUUM DEPRESSIONS

被引：16

作者：

AURASS, H

HOFMANN, A

MAGUN, A

SORUESCAUT, I

ZLOBEC, P

机构：

[1] UNIV BERN,INST ANGEW PHYS,CH-3012 BERN,SWITZERLAND

[2] OBSERV PARIS,ASTROPHYS SECT,F-92195 MEUDON,FRANCE

[3] OSSERV ASTRON TRIESTE,I-34131 TRIESTE,ITALY

来源：

SOLAR PHYSICS | 1993年 / 145卷 / 01期

关键词：

D O I：

10.1007/BF00627991

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the active region NOAA 6718 and the development of a (2N, M3.6) flare in radio and Halpha. Due to our knowledge of the magnetic field structure in the active region we are able to associate the different radio flare burst components with the stages in the Ha flare evolution. A discussion of the data in terms of chromospheric flare kernel heating reveals that in the present case the observed flare-related radio burst continuum switch-off is caused by the penetration of hot, ablated ps into the coronal radio source.

引用

页码：151 / 168

页数：18

共 11 条

[1] FIBER BURSTS IN TYPE-IV DM RADIO CONTINUA AS A SIGNATURE OF CORONAL CURRENT SHEET DYNAMICS [J].