A conjectured pulsar magnetosphere model

Details A conjectured pulsar magnetosphere model A conjectured pulsar magnetosphere model

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssct....4...91b&link_type=abstract

Speculations in Science and Technology, vol. 4, Apr. 1981, p. 91-97.

Physics

3

Energy Dissipation, Magnetohydrodynamic Flow, Pulsar Magnetospheres, Pulsars, Stellar Models, Angular Momentum, Flow Distribution, Particle Emission, Particle Energy, Poloidal Flux, Stellar Magnetic Fields

Scientific paper

A pulsar magnetosphere model is proposed in which the characteristic feature is the existence of dissipative 'collars' around each pole. Particles emitted from the star lose energy in infinite gradients of their Lorentz factors and azimuthal speeds and return to the star. A sketch of a flow diagram showing typical flow curves in the proposed model is included.

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