High angular resolution radio observations of the outer solar corona

被引：0
|
作者：
Ramesh, R [1 ]
Subramanian, KR [1 ]
Sastry, CV [1 ]
机构：
[1] Indian Inst Astrophys, Bangalore 560034, Karnataka, India
来源：
CORONAL STRUCTURE AND DYNAMICS NEAR SOLAR ACTIVITY MINIMUM | 2000年 / 25卷 / 09期
关键词：
D O I：
10.1016/S0273-1177(99)00596-7
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
We report high angular resolution observations of the outer solar corona carried out at 75 MHz from the Gauribidanur Radio Observatory (Long: 77 degrees 26/12 " E, Lat: 13 degrees 36'12 " N) about 100 km north of Bangalore, India, during the solar eclipse of October 24, 1995. Our main conclusion is that there are structures of angular size less than or equal to 2.5' in the outer solar corona at a height of approximate to 0.4 R. above the photosphere. (C) 2000 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：1847 / 1850
页数：4
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