Positional drift within groups of Type I solar radio bursts

Details Positional drift within groups of Type I solar radio bursts Positional drift within groups of Type I solar radio bursts

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103..129v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 103, Jan. 1986, p. 129-140.

Physics

3

Angular Distribution, Solar Radio Bursts, Position (Location), Radio Interferometers, Radio Spectra

Scientific paper

In the dynamic spectrograms of the 60-channel solar radiospectrograph at Dwingeloo coherent groups of Type I bursts have been selected. At 243 MHz the positions of the bursts were measured. Within many groups the bursts showed a systematic angular displacement with time. Movements with apparent velocities up to 15000 km s-1 have been observed. The burst positions have been obtained with a two-element interferometer. A special data reduction method used the amplitude variation of the Type I bursts as a parameter for selection against the background radiation.

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