Pulsar magnetosphere with conspicuous trans-field flow

Details Pulsar magnetosphere with conspicuous trans-field flow Pulsar magnetosphere with conspicuous trans-field flow

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..105s&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Atmospheric Circulation, Magnetohydrodynamic Flow, Pulsar Magnetospheres, Pulsars, Electric Fields, Electromagnetic Fields, Stellar Models

Scientific paper

While it is widely known that no self-consistent model of a pulsar magnetosphere can be constructed under the ideal-MHD condition, the reason for this (and for the real global structure of the magnetosphere) is not clear. It is presently shown that, in the pulsar magnetosphere, the violation of the ideal MHD condition by conspicuous transfield motion and nonzero field-aligned electric field is due to relativistic large inertia. In addition, an axisymmetric numerical model with tenuous plasma suggests that a vacuum-like electric field and a closed current circuit develop in the region of the transfield flow.

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