Scattering of pulsar radiation by turbulent interstellar plasma

Details Scattering of pulsar radiation by turbulent interstellar plasma Scattering of pulsar radiation by turbulent interstellar plasma

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55...69b&link_type=abstract

Astronomicheskii Zhurnal, vol. 55, no. 1, 1978, p. 69-75. In Russian. (Translation).

Astronomy and Astrophysics

Astronomy

Cosmic Plasma, Electromagnetic Scattering, Plasma Turbulence, Plasma-Electromagnetic Interaction, Pulsars, Amplitudes, Interstellar Matter, Signal Transmission, Stochastic Processes, Transport Theory

Scientific paper

Stochastic transport theory is applied to the solution of the problem of the propagation of a pulsar signal in a turbulent interstellar plasma. Results of the theory are used to predict the amplitude fluctuations of pulsar radiation and the frequency correlation of the signal. Theoretical results are compared with a few available experimental results and are used to determine the mean scale of turbulence.

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