An algorithm for solving the pulsar equation
نویسندگان
چکیده
We present an algorithm of finding numerical solutions of pulsar equation. The problem of finding the solutions was reduced to finding expansion coefficients of the source term of the equation in a base of orthogonal functions defined on the unit interval by minimizing a multi-variable mismatch function defined on the light cylinder. We applied the algorithm to Scharlemann & Wagoner boundary conditions by which a smooth solution is reconstructed that by construction passes successfully the Gruzinov’s test of the source function exponent.
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ورودعنوان ژورنال:
- CoRR
دوره abs/astro-ph/0605514 شماره
صفحات -
تاریخ انتشار 2006