Radiation phenomena in type II solar radio bursts and laboratory shock-wave experiments

Details Radiation phenomena in type II solar radio bursts and laboratory shock-wave experiments Radiation phenomena in type II solar radio bursts and laboratory shock-wave experiments

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..500k&link_type=abstract

Astrophysical Journal, vol. 199, July 15, 1975, pt. 1, p. 500-503. Research supported by the John Simon Guggenheim Memorial Fou

Astronomy and Astrophysics

Astrophysics

7

Collisionless Plasmas, Plasma Heating, Shock Wave Interaction, Type 2 Bursts, Electron Distribution, Energy Spectra, Magnetohydrodynamic Stability, Plasma Turbulence, Solar Corona

Scientific paper

The known spectrum of turbulence in and behind a collisionless shock wave is used to compute the relaxation of the electron distribution function in the presence of that turbulent spectrum. It is concluded that a nonthermal tail of the sort required to explain type II solar burst radiation does not develop from the turbulent environment of a collisionless shock wave. Alternate mechanisms for the radiation are proposed, based on similar observations in laboratory experiments.

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