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Drifting Subpulses in Pulsars

Published online by Cambridge University Press:  25 April 2016

Michelle C. Allen  and
D. B. Melrose
Michelle C. Allen
Affiliation:
School of Physics, University of Sydney
D. B. Melrose
Affiliation:
School of Physics, University of Sydney
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Extract

Individual pulses from a given pulsar can differ greatly in both shape and intensity, and are often made up of narrower ‘subpulses’, i.e. local emission peaks one tenth the width of the mean pulse. Properties such as shape, polarization and position of subpulses presumably reflect details of the emission processes and of the regions that produce the radiation.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 191 - 195
Copyright
Copyright © Astronomical Society of Australia 1983

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