Physics
Scientific paper
Apr 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6r..66i&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Mar.-Apr. 1990, p. 66-69. In Russian.
Physics
Magnetohydrodynamic Waves, Plasma Dynamics, Solar Radio Emission, Electromagnetic Radiation, Electron Distribution, Type 2 Bursts, Type 3 Bursts
Scientific paper
The influence of sporadic solar radio emission on the dispersion properties of kinetic Alfven waves is studied. It is shown that the electromagnetic wave changes the electron distribution function and leads to an electron drift of the related ions. If the amplitude of the electromagnetic waves is sufficiently high, the kinetic Alfven wave instability occurs. It is found that the power of the sporadic radio emission during type I and II solar radio bursts is sufficient to generate the kinetic Alfven wave excitation. It is concluded that Landau damping of the kinetic Alfven waves causes the heating of the coronal plasma.
Iukhimuk A. K.
Kuts S. V.
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