Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..270f&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, March 1990, p. 270-278. In Russian. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
2
Light Emission, Particle Acceleration, Shock Wave Propagation, Synchrotron Radiation, Magnetohydrodynamic Turbulence, Polarization (Waves), Radiation Spectra
Scientific paper
It is shown that the acceleration of electrons needed for the generation of synchrotron radiation in the optical range can be provided by shock waves if a self-consistent regime of Alfven wave generation exists. The turbulence level near the front is evaluated, and the possibility of directly studying this turbulence level on the basis of radiation spectrum and polarization at frequencies greater than the cutoff frequency is discussed. A correlation between alpha and the cutoff frequency is predicted. It is suggested that the turbulence is not self-consistent if this correlation is not present.
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