On a sequence of remarkable fine structures in the type IV burst of 24 April, 1985

Details On a sequence of remarkable fine structures in the type IV burst of 24 April, 1985 On a sequence of remarkable fine structures in the type IV burst of 24 April, 1985

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..347a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 112, no. 2, 1987, p. 347-357.

Physics

22

Continuous Spectra, Emission Spectra, Fine Structure, Solar Spectra, Stellar Models, Type 4 Bursts, Solar Flares, Spectrum Analysis, Whistlers

Scientific paper

During the type IV burst on 24 April, 1985 the authors observed at 234 MHz an untypical, strong, nearly six hours lasting continuum emission incorporating several groups of braodband pulsations, zebra patterns, fiber bursts, and a new fine structure phenomenon. The power spectra of the groups of broadband pulsations reveal no simple structure. There is only one common periodic component between 0.3 s and 0.4 s. Slowly drifting chains of narrowband fiber bursts are described as a new fine structure by spectrograms and simultaneously recorded single frequency intensity profiles. A qualitative model of this new fine structure is suggested.

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