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Drifting Subpulses in Pulsars
Published online by Cambridge University Press: 25 April 2016
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.
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- Copyright © Astronomical Society of Australia 1983
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