Confirmation of quiet pulsar model by the boundary element method

Details Confirmation of quiet pulsar model by the boundary element method Confirmation of quiet pulsar model by the boundary element method

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..187s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 2, Nov. 1989, p. 187-194.

Statistics

Computation

7

Boundary Element Method, Computational Astrophysics, Pulsars, Stellar Magnetospheres, Stellar Models, Toroidal Plasmas, Boundary Value Problems, Charged Particles, Magnetic Dipoles, Mathematical Models, Polarization (Charge Separation)

Scientific paper

A method for solving the force-free surface problem for the pulsar magnetosphere is outlined. The given formulation is extended to an oblique rotator problem. The boundary element method developed in Paper I is used - to directly determine the force-free surface. Another merit of this method rests in the fact that only a two-dimensional grid is used, in spite of the problem being three-dimensional. A numerical calculation has been performed to confirm the solution by the particle method (Krause-Polstorff and Michel, 1985).

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