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Frequency Structure of Radio Scintillations for Several Pulsars

Published online by Cambridge University Press:  12 April 2016

V.I. Kondratiev ,
M.V. Popov ,
V.A. Soglasnov  and
S.V. Kostyuk
V.I. Kondratiev
Affiliation:
Astro Space Center, Profsoyuznaya str., 84/32, Moscow 117997, Russia. E-mail: vlad@tanatos.asc.rssi.ru
M.V. Popov
Affiliation:
Astro Space Center, Profsoyuznaya str., 84/32, Moscow 117997, Russia. E-mail: vlad@tanatos.asc.rssi.ru
V.A. Soglasnov
Affiliation:
Astro Space Center, Profsoyuznaya str., 84/32, Moscow 117997, Russia. E-mail: vlad@tanatos.asc.rssi.ru
S.V. Kostyuk
Affiliation:
Astro Space Center, Profsoyuznaya str., 84/32, Moscow 117997, Russia Moscow State University, Vorobievy Hills, Moscow 119899Russia

Abstract

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Scintillation times and decorrelation bandwidths for the pulsars B0329+54, B1641-15, B1508+55 and B1919+21 are determined. The results are based on observations made with different instruments and at different radio frequencies. All objects but the pulsar B1508+55 were detected to have more than one frequency scale. The obtained values of scattering parameters are not contrary in general to the Kkolmogorov form of density fluctuation spectrum.

Type
Chapter Two Pulsars: Their Scattering and Intrinsic Properties
Information
International Astronomical Union Colloquium , Volume 182: Sources and Scintillations: Refraction and Scattering in Radio Astronomy , 2001 , pp. 43 - 46
Copyright
Copyright © Kluwer 2001

References

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Popov, M.V. and Soglasnov, V.A.: 1984, Observations of Interstellar Scattering of Radio Emission of Pulsar PSR 0329+54 at 102.5 MHz, Soviet Astron. 28, 424–427.Google Scholar