The nature of fluctuations of the solar radio emission of type I noise storms

Details The nature of fluctuations of the solar radio emission of type I noise storms The nature of fluctuations of the solar radio emission of type I noise storms

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..704g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Aug. 1987, p. 704-709. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Noise Storms, Periodic Variations, Solar Radio Bursts, Solar Radio Emission, Solar Storms, Coronal Loops, Plasma Oscillations, Radiant Flux Density, Solar Wind

Scientific paper

A possible mechanism of fluctuations and quasi-periodic variations of intensity of solar radio noise storms is discussed. The mechanism is based on the development of relaxation oscillations of plasma parameters in adiabatic traps which are the coronal magnetic loops. The power of energetic particle sources in radio sources is estimated using the observed period of radio emission variations.

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