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An Auroral Model for Particle Acceleration in Pulsars



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Recording Details

Speaker(s): 
Collection/Series: 
PIRSA Number: 
10100000

Abstract

I discuss a model for particle acceleration in the current sheet separating the open and closed field line regions, and crossing the
neutral line region, of a pulsar's magnetosphere, which has substantial kinship to the phenomena observed in planetary magnetospheres within the solar system. Possible applications to gamma ray emission from pulsars are also described.