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Whence the pulses?

Published online by Cambridge University Press:  12 April 2016

D.B. Melrose
D.B. Melrose*
Affiliation:
School of Physics, University of Sydney, NSW 2006, AUSTRALIA

Abstract

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Radio emission mechanisms for pulsars are reviewed with emphasis on five possible sites for the emission: the pair production front (PPF), two regions in the relativistically outflowing plasma (denoted ROP1 and ROP2) between the PPF and the light cylinder (LC), and two sited near the LC. Several maser emission mechanism are viable for ROP1, where radius-to-frequency mapping applies. Suggested Schott radiation from outside the LC is discussed critically.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 139 - 146
Copyright
Copyright © Astronomical Society of the Pacific 1996

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