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- W43389108 abstract "The stochastic transport theory originally developed by the author for the study of electromagnetic wave propagation in media characterized by a random-phase velocity is applied to the problem of the propagation of a pulsar signal through the turbulent interstellar plasma. The theoretical results are used to predict the amplitude fluctuations of pulsar radiation and the coherence of pulsar signals in the frequency domain. A comparison is made with a few experimental data. The mean scale of the turbulence is estimated. Analysis of this kind can not only elucidate the effects of the interstellar medium on pulsar characteristics but it can aid us in understanding the medium itself. Future extensions of the theory could be applied to improve the design of large-scale radio astronomy systems using adaptive receivers in searches for encoded signals generated by extraterrestrial civilizations." @default.
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- W43389108 date "1978-01-01" @default.
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- W43389108 title "Multiple scattering of pulsar signals by turbulent interstellar plasma" @default.
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