The axisymmetric pulsar magnetosphere. II

Details The axisymmetric pulsar magnetosphere. II The axisymmetric pulsar magnetosphere. II

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.188..799m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 188, Sept. 1979, p. 799-812.

Astronomy and Astrophysics

Astronomy

36

Pulsar Magnetospheres, Pulsars, Stellar Magnetic Fields, Stellar Models, Boundary Value Problems, Fourier Transformation, Gaps, Light Speed, Michell Theorem, Stellar Rotation

Scientific paper

A Fourier transform method is presented for the construction of model pulsar magnetic fields. The method can be employed as part of an iterative scheme for the construction of a self-consistent magnetosphere. Three illustrative models are computed, for which respectively: (1) the entire region as far as the light-cylinder consists of massless corotating charges; (2) some of the corotating ions are removed to produce a thin gap near the light-cylinder; (3) a large wedge of ions is removed.

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