Numerical study of jets produced by conical wire arrays on the Magpie pulsed power generator

Details Numerical study of jets produced by conical wire arrays on the Magpie pulsed power generator Numerical study of jets produced by conical wire arrays on the Magpie pulsed power generator

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..429b&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 429-432

Astronomy and Astrophysics

Astrophysics

Ism: Jets And Outflows, Hydrodynamics, Plasmas, Methods: Laboratory, Methods: Numerical

Scientific paper

With the aim to model jets produced by conical wire arrays on the MAGPIE generator, and to strengthen the link between laboratory and astrophysical jets, we performed three-dimensional magneto-hydro-dynamic numerical simulations using the code GORGON and successfully reproduced the experiments. We found that a minimum resolution of ~100 μm is required to retrieve the unstable character of the jet. Moreover, arrays with less wires produce more unstable jets with stronger magnetic fields around them.

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