Supersonic jet production in conical wire array Z-pinches
is modeled using a two-dimensional (2D) resistive
magneto-hydrodynamic (MHD) code. In conical wire arrays, the
converging plasma ablated from the wires stagnates on axis,
forming a standing conical shock which redirects and collimates
the flow into a jet. As the jet exits the collimator shock,
it is radiatively cooled and accelerated by the steep thermal
gradients present. Purely hydrodynamic simulations using conditions
relevant to the MAGPIE facility show good agreement with the
experiments (Lebedev et al., 2002), indicating that
narrow, high Mach number (M ∼ 20), radiatively cooled
tungsten jets of astrophysical relevance can be obtained. To
investigate the effects of lower radiative cooling on jet collimation,
we modeled an aluminum conical wire array. When radiative losses are
less significant, lower Mach number (M ∼ 10), less collimated
jets are obtained. MHD simulations relevant to the “Z”
facility were carried out to investigate the scaling of jet parameters.
The resulting hypersonic (M ∼ 40), high density jets should
allow the investigation of a wider range of astrophysical jet conditions.