A numerical method to determine the electromagnetic field of the pulsar magnetosphere with inclined magnetic moment

Statistics – Computation

Scientific paper

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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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