Keywords: MHD, ideal plasma instabilities
zPinch
The Z-Pinch is an ideal MHD simulation of a cylindrical plasma with a purely axial current and a periodic boundary condition in the axial direction. This problem uses a top-hat current density profile such that
where \(r_p\) is the current column radius. Thus, the magnetic field is
The MHD force balance condition (\(\mathbf{J}\times\mathbf{B}=\nabla p\)) becomes
and, thus, the pressure profile is
where \(\alpha\) sets the base pressure outside the plasma column.
In general, the plasma column may be unstable to perturbations with a wavenumber (\(\mathbf{k}\)) such that
where \(m\) is the azimuthal wavenumber, \(n\) is the axial wavenumber, and \(Z\) is the axial length of the computational domain. This example assumes axisymmetry in the azimuthal direction of the cylindrical column, and thus instabilities with \(m=0\) are modeled. The simulation is initialized with a \(n=1\) perturbation in the magnetic field which leads to instability with the default parameters.
This simulation can be performed with a USimBase license.
The Unstable Plasma Z-Pinch example is accessed from within USimComposer by the following actions:
The basic example variables are editable in the Editor pane of the Setup window as described below. After any change is made, the Save and Process Setup button must be pressed again before a new run may commence.
The key variables of the input file are exposed in the Setup window. These variables allow one to set the following fields:
The following parameters control the physics of the Z-Pinch:
The following parameters control the dimensionality, domain size and resolution of the simulation:
The following parameters the length of the simulation and data output:
The following parameters control the USim solvers used to evolve the Z-Pinch:
After performing the above actions, continue as follows:
You will also see the engine log output in the Logs and Output Files pane. The run has completed when you see the output, “Engine completed successfully.”
After performing the above actions, continue as follows:
The plot in Fig. 81 was made with the calewhite color scale at time \(3\times10^{-6}\) seconds. Here the instability is in the nonlinear phase, and the plasma density has ruptured out of the initial plasma column.