Statistics – Computation
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..145s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 1, Nov. 1989, p. 145-158.
Statistics
Computation
5
Computational Astrophysics, Electromagnetic Fields, Magnetic Moments, Pulsar Magnetospheres, Fourier Transformation, Iterative Solution, Magnetohydrodynamics, Particle Acceleration
Scientific paper
A numerical method to determine the electromagnetic field of a steadily rotating magnetosphere with an inclined magnetic moment under a given boundary condition on an arbitrary shaped boundary surface is presented. The region may include the light cylinder. The present method, together with a companion method giving particle motion and creation, makes an iterative scheme to obtain a global model of the pulsar magnetosphere. A key problem in explaining the particle acceleration in pulsars is to solve field-aligned electric field in an accelerating region bounded by an ideal-MHD region. The present method is fit to connect a solution for the nonideal-MHD region with another solution for the ideal-MHD region on a boundary surface whose location should also be solved.
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