Electric gaps in pulsar magnetospheres

Details Electric gaps in pulsar magnetospheres Electric gaps in pulsar magnetospheres

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...68..337m&link_type=abstract

Space Science Reviews, Volume 68, Issue 1-4, pp. 337-348

Computer Science

2

Scientific paper

Two contrasting models of the magnetosphere are studied: a classical, quasi-mhd model, in which it is the componentE ⊥ that accelerates electrons to relativistic energies; and a model with e+-e- production, in which the componentE ∥ is locally crucial, both in an acceleration domain near the star and in a dissipation domain beyond the light-cylinder.

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