An emission mechanism explaining off-pulse emission originating in the outer magnetosphere of pulsars
classification
🌌 astro-ph.HE
keywords
emissionoff-pulseinstabilitymagnetospheremechanismplasmapulsarscondition
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We have examined the cyclotron resonance instability developing in the relativistic out-flowing plasma in the pulsar magnetosphere. The instability condition leads to radio emission in the sub-GHz frequency regime which is likely to be seen as off-pulse emission. Recent studies have shown the presence of off-pulse emission in long period pulsars, and we demonstrate this plasma process to be an energetically viable mechanism.
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