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arXiv · 0804.4176

Dissipative Pulsar Magnetosphere

Andrei Gruzinov
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Abstract

Dissipative axisymmetric pulsar magnetosphere is calculated by a direct numerical simulation of the Strong-Field Electrodynamics equations. The magnetic separatrix disappears, it is replaced by a region of enhanced dissipation. With a better numerical scheme, one should be able to calculate the bolometric lightcurves for a given conductivity.

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Andrei Gruzinov. 2008-10-02. Dissipative Pulsar Magnetosphere. https://doi.org/10.1088/1475-7516%2F2008%2F11%2F002

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