Solar Millisecond Spikes Manifest Large- and Small-Scale Inhomogeneities of the Coronal Plasma

Details Solar Millisecond Spikes Manifest Large- and Small-Scale Inhomogeneities of the Coronal Plasma Solar Millisecond Spikes Manifest Large- and Small-Scale Inhomogeneities of the Coronal Plasma

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47..129k&link_type=abstract

Astronomy Reports, vol. 47, Issue 2, p.129-138

Astronomy and Astrophysics

Astronomy

2

Scientific paper

A model for the generation of solar millisecond radio spikes via a maser cyclotron resonance is proposed. The model takes into account the large-scale inhomogeneity of the magnetic field and small-scale inhomogeneities of the coronal plasma. The efficiency of the energy transformation from a electron beam into maser radiation is estimated. Appropriate parameters of the magnetic field inhomogeneity and the plasma turbulence are found.

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