The maser mechanism for solar millisecond spike generation in inhomogeneous plasma

Details The maser mechanism for solar millisecond spike generation in inhomogeneous plasma The maser mechanism for solar millisecond spike generation in inhomogeneous plasma

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...382.1061v&link_type=abstract

Astronomy and Astrophysics, v.382, p.1061-1069 (2002)

Astronomy and Astrophysics

Astrophysics

11

Sun: Flares, Sun: Radio Radiation, Sun: Particle Emission, Masers

Scientific paper

The generation of solar millisecond spikes on the maser cyclotron resonance is studied by taking into account the large-scale monotonic magnetic field inhomogeneity and the small-scale plasma inhomogeneity. It is shown that the presence of these inhomogeneities can have a significant effect on the generation of electromagnetic waves. In this case the structure of the inhomogeneities determines the spectral and temporal parameters of emission. A modeling of the spike dynamic spectrum in the presence of a small-scale inhomogeneity of coronal plasma is performed. It is shown that a simple model of the plasma inhomogeneity (traveling density wave) can account for many of the observed features of spikes.

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