The Cherenkov effect and plasma turbulent reactors

Details The Cherenkov effect and plasma turbulent reactors The Cherenkov effect and plasma turbulent reactors

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap.....18..641l&link_type=abstract

(Astrofizika, vol. 18, Oct.-Dec. 1982, p. 641-650) Astrophysics (ISSN 0571-7132), vol. 18, no. 4, April 1983, p. 367-373. Transl

Astronomy and Astrophysics

Astronomy

Cerenkov Radiation, Extraterrestrial Radio Waves, Plasma Radiation, Plasma Turbulence, Compton Effect, Cosmic Plasma, Distribution Functions, Radio Sources (Astronomy), Relativistic Particles

Scientific paper

The restrictions governing the energy interval of the power-law distribution function for the relativistic electrons formed in a plasma turbulent reactor (Tsytovich and Chukhachev, 1969) from the Cerenkov effect and ionization losses are determined. A determination is also made of the curvature signs in the distortions of the distribution function at low energies. The possibility of interpreting features in the radiation spectra of cosmic radio sources in the decameter wavelength range is considered. It is assumed that Langmuir turbulence is maintained in the reactor at a constant level by a source of sufficient power.

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