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Propagation of radio waves in pulsar magnetospheres

Published online by Cambridge University Press:  12 April 2016

S.A. Petrova  and
Yu.E. Lyubarskii
S.A. Petrova
Affiliation:
Institute of Radio Astronomy, 4 Chervonopraporna Str., Kharkiv, 310002, Ukraine
Yu.E. Lyubarskii
Affiliation:
Institute of Radio Astronomy, 4 Chervonopraporna Str., Kharkiv, 310002, Ukraine

Abstract

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The morphological classification of pulsar profiles is interpreted within the frame of the primordial hollow-cone emission model taking into account wave propagation in the magnetosphere. In this context the frequency evolution of the profiles as well as the difference in polarization properties of core and conal components can be explained naturally.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 403 - 404
Copyright
Copyright © Astronomical Society of the Pacific 2000

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