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

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

Jun 1975

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

Fizika Plazmy, vol. 1, May-June 1975, p. 436-440. In Russian.

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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