Decay of type III radio bursts in the solar corona

Details Decay of type III radio bursts in the solar corona Decay of type III radio bursts in the solar corona

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1..149g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, July 1975, p. 34-38.) Soviet Astronomy Letters, vol. 1, July-Aug. 1975, p. 149, 150.

Physics

Landau Damping, Plasma Waves, Solar Corona, Type 3 Bursts, Decay Rates, Plasma Density, Plasmons, Radio Attenuation, Solar Physics, Solar Wind Velocity

Scientific paper

The decay of low frequency type III bursts cannot be explained by Landau damping at the nonthermal tail of the one-dimensional electron-velocity distribution in the coronal plasma. The abrupt cutoff of burst intensity by Landau damping due to the coronal density gradient is probably prevented by the induced scattering of plasma waves on ions, which creates a plasmon flux in the direction of the increase in plasma density.

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