ZEBRA pattern flux density observation during the type IV burst on October 12, 1981

Details ZEBRA pattern flux density observation during the type IV burst on October 12, 1981 ZEBRA pattern flux density observation during the type IV burst on October 12, 1981

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...84..339a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 84, April 1983, p. 339-345.

Physics

8

Continuous Spectra, Fine Structure, Flux Density, Radio Spectra, Type 4 Bursts, Absorption Spectra, Emission Spectra, Extremum Values, Histograms, Whistlers

Scientific paper

A new quantitative zebra pattern observation is reported. The mean amplitude ratio of the emission and absorption features of the irregular zebra pattern observed simultaneously with and related to an increased continuum is Q = 3. This is not contradictory to a zebra pattern model in terms of whistler soliton propagation throughout the source of continuum emission.

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