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Pulsar Microstructure Quasi-Periodicity

Published online by Cambridge University Press:  14 August 2015

Valentin Boriakoff ,
Dale C. Ferguson  and
Gregory Slater
Valentin Boriakoff
Affiliation:
NAIC, Cornell University, Ithaca, NY
Dale C. Ferguson
Affiliation:
NAIC, Arecibo Observatory, Arecibo, PR
Gregory Slater
Affiliation:
Cornell University, Ithaca, NY

Abstract

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Microstructure in pulsars occasionally has a quasi-periodic character with an average period of around 0.9 ms. A survey of this little known phenomenon (time characteristics, polarization, frequency behaviour, etc.) together with some new results are presented. Some physical interpretations (e.g. vibration of the neutron star, polar cap periodical sparking, standing wave pattern in the velocity of light cylinder model) are also presented.

Type
III. Radio Observations of Pulsars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 199 - 204
Copyright
Copyright © Reidel 1981 

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