A self-modulation model of solar radio emission

Details A self-modulation model of solar radio emission A self-modulation model of solar radio emission

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acasn..38..379w&link_type=abstract

Acta Astronomica Sinica, vol. 38, p. 379

Astronomy and Astrophysics

Astronomy

Solar Radio Emission, Electromagnetic Wave Transmission, Solar Corona, Solar X-Rays, Solar Radio Bursts, Astronomical Models, Modulation, Systems Stability, Nonlinear Equations

Scientific paper

The existing theoretical model of self-modulation instability in the nonlinear waves propagation is adopted in this work. We want to investigate the possibility of self-modulation instabilities occurring in the electromagnetic waves propagating in the solar corona. It is found that only decimeter and meter radio bursts can produce the longitudinal and transverse self-modulation instabilities in the outer corona and that the optical, X-ray, and high frequency electromagnetic waves are unable to produce such modulation processes. This theoretical model is consistent with the observed fine structures of solar meter wave bursts.

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