A note on the emission mechanism of storm radiation

Details A note on the emission mechanism of storm radiation A note on the emission mechanism of storm radiation

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..126..367g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 126, April 1990, p. 367-370.

Physics

1

Noise Storms, Solar Flares, Solar Radio Bursts, Plasma Waves, Radio Emission

Scientific paper

A new mechanism has been proposed for the continuum and burst components of solar storm radiation by Genkin et al. (1989). It is suggested that, while bursts can be explained by the proposed mechanism of scattering on plasma turbulence generated density fluctuations, the continuum cannot be explained by scattering on thermal ion density fluctuations. Second harmonic emissions will dominate over the fundamental emission due to scattering on thermal ion density fluctuations in contradiction to observations.

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