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A Resonant-Mode Model of Pulsar Radio Emission

Published online by Cambridge University Press:  19 July 2016

M. D. T. Young
M. D. T. Young*
Affiliation:
School of Physics, University of Western Australia, 35 Stirling Highway, Crawley WA 6009, Australia

Abstract

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It is argued that the polar gap and flux tube in the pulsar magnetosphere act as a resonant cavity/waveguide system which is excited by oscillations in the primary beam current and accelerating potential. The modes will be converted, probably scattered, to produce radio beams in the frequency range of those observed.

Type
Part 8: Pulsar Electrodynamics and Emission Theory
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 365 - 368
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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