Analysis of the modulation depth in fast pulsations of solar radio emission

Details Analysis of the modulation depth in fast pulsations of solar radio emission Analysis of the modulation depth in fast pulsations of solar radio emission

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1026c&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Sept.-Oct. 1990, p. 1026-1037. In Russian.

Astronomy and Astrophysics

Astronomy

1

Solar Radio Emission, Solar Spectra, Temporal Distribution, Type 4 Bursts, Astronomical Models, Magnetohydrodynamic Stability, Whistlers

Scientific paper

A statistical analysis of the modulation depth in five type IV bursts confirms a model of millisecond pulsations of radio emission due to a pulsation regime of the whistler spectrum. The modulation depth distribution (Delta I)/I versus the period p grows linearly (with different slope) up to the maximum at (Delta I)/I = 0.5-0.6 for p = 1/nu(ei). The same dependence (Delta I)/I (p) for spikes observed in the same phenomena also tends to confirm this model.

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