Structure of the magnetosphere of a rotating star

Details Structure of the magnetosphere of a rotating star Structure of the magnetosphere of a rotating star

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9...71b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 2, p. 71-81.

Physics

Lines Of Force, Pulsars, Stellar Magnetic Fields, Stellar Magnetospheres, Stellar Rotation, White Dwarf Stars, Atmospheric Models, Magnetic Dipoles, Pulsar Magnetospheres

Scientific paper

The structure of the quasi-stationary magnetosphere of an oblique rotator in the region of closed magnetic field lines is considered. The structure and appearance of vacuum gaps at a zero corotation charge surface for arbitrary magnetic dipole slopes and distances to the star are investigated. The possibility of existence of local quasi-neutral high density plasma inhomogeneities is studied. These phenomena for pulsars and white dwarfs are discussed.

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