Three-dimensional ordinary-wave soliton and type I solar radio bursts

Details Three-dimensional ordinary-wave soliton and type I solar radio bursts Three-dimensional ordinary-wave soliton and type I solar radio bursts

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975svjpp...1r.436k&link_type=abstract

(Fizika Plazmy, vol. 1, May-June 1975, p. 436-440.) Soviet Journal of Plasma Physics, vol. 1, May-June 1975, p. 241-243. Transl

Physics

Plasma Physics

Plasma Radiation, Solar Corona, Solar Radio Bursts, Solar Wind, Solitary Waves, Magnetohydrodynamic Stability, Plasma Dynamics, Polarized Radiation, Pulsed Radiation

Scientific paper

The potential well involved in type I radio bursts is found to be a three-dimensional soliton of an ordinary wave. The maximum energy density at which such a soliton can still exist is estimated. It is shown that clusters consisting of a large number of these solitons may be formed by a plasma instability in the corona. It is noted that this phenomenon can explain the basic properties of type I radio bursts, including their pulsed nature, narrowband characteristics, polarization, and emission direction.

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