Electromagnetics in rotation-powered pulsar

Details Electromagnetics in rotation-powered pulsar Electromagnetics in rotation-powered pulsar

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..250a&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 4, p. 250 - 256 (2005)

Astronomy and Astrophysics

Astronomy

Pulsars, Magnetospheres

Scientific paper

An electric field parallel to the magnetic field line in the pulsar magnetosphere leads to the pulsar wind. We explain difficulties to establish a model with a consistent electric field. If there is a proton counterflow in the magnetosphere, it can provide an anode to make such an electric field. In addition, the proton counterflow is suitable for reproducing bright radio emission from pulsars.

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