An Auroral Model for Particle Acceleration in Pulsars



Playing this video requires the latest flash player from Adobe.

Download link (right click and 'save-as') for playing in VLC or other compatible player.


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.