Magnetospheric launching in resistive MHD simulations

Details Magnetospheric launching in resistive MHD simulations Magnetospheric launching in resistive MHD simulations

2011-10-26

arxiv.org/abs/1110.5699v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

2 pages, 3 figures, to appear: in Proceedings of MFU III conference held in August, 2011 in Zakopane, Poland

Scientific paper

We perform numerical simulations in the close vicinity of a slowly rotating young stellar object. Using our own resistive MHD Zeus347 code in 2D axisymmetry, magnetospheric interaction experiences four robust stages in evolution. Quasi-stationary axial and conical streams of outflowing matter can last many orbital periods as results of the resistivity-facilitated magnetic reconnections. The shape of the magnetic field depends on resistivity in the magnetosphere.

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