Association of type II soalr radio bursts with coronal structures above H-alpha filament channels

Details Association of type II soalr radio bursts with coronal structures above H-alpha filament channels Association of type II soalr radio bursts with coronal structures above H-alpha filament channels

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...94..379s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 94, Sept. 1984, p. 379-385.

Physics

12

H Alpha Line, Solar Corona, Solar Prominences, Type 2 Bursts, Solar Flares, Solar Magnetic Field, Statistical Tests, Ultrahigh Frequencies

Scientific paper

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 Hα filaments rather than above Hα flares. This suggests that the type II radio emission most probably originates from within a coronal helmet streamer overlying the filament channel.

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