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Radiation from Pulsars
Published online by Cambridge University Press: 07 February 2017
Abstract
We suggest that an oscillating interface, carrying a steady current between a rotating, radiating, magnetic dipole and an external plasma is the source of pulsar radiation produced over a broad band of high frequencies (108–1018 Hz). The efficiency of the radiation mechanism is so high that the oscillation energy goes mainly into radiation in each cycle of the oscillation.
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- Copyright © Reidel 1971