On the construction of a simple model pulsar magnetosphere

Details On the construction of a simple model pulsar magnetosphere On the construction of a simple model pulsar magnetosphere

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.254..355m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 254, Jan. 15, 1992, p. 355-360.

Statistics

Computation

16

Computational Astrophysics, Pulsar Magnetospheres, Stellar Models, Eigenvalues, Fourier Transformation, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

The simplest example illustrating the effect of magnetospheric charges on a pulsar magnetic field has the region within the light cylinder filled with the Goldreich-Julian charge density which corotates with the star. It is shown that two superficially different techniques for constructing the magnetic field are formally equivalent. The relative advantages of each representation are briefly discussed.

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