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We have examined the cyclotron resonance instability developing in therelativistic out-flowing plasma in the pulsar magnetosphere. The instabilitycondition leads to radio emission in the sub-GHz frequency regime which islikely to be seen as off-pulse emission. Recent studies have shown the presenceof off-pulse emission in long period pulsars, and we demonstrate this plasmaprocess to be an energetically viable mechanism.

An emission mechanism explaining off-pulse emission originating in the outer magnetosphere of pulsars