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Association of type II solar radio bursts with coronal structures above Hα filament channels

✍ Scribed by R. T. Stewart


Publisher
Springer
Year
1984
Tongue
English
Weight
316 KB
Volume
94
Category
Article
ISSN
0038-0938

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✦ Synopsis


A study of type II solar radio bursts recorded at 160 MHz by the Culgoora radioheliograph during 1980 to 1982 shows that the radio emission occurs above He filaments rather than above He flares. This suggests that the type II radio emission most probably originates from within a coronal helmet streamer overlying the filament channel.