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Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields
Authors:Andrea Mignone  Silvano Massaglia  Gianluigi Bodo
Institution:(1) Dipartimento di Fisica Generale dell’Università, Via Pietro Giuria 1, I-10125 Torino, Italy;(2) Osservatorio Astronomico di Torino, Viale Osservatorio 20, I-10025 Pino Torinese, Italy
Abstract:This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach.
Keywords:magnetohydrodynamics  methods: numerical  relativity  shock waves  galaxies: active  galaxies: jets
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