MHD Simulations on Magnetic Compression of Field Reversed Configurations

TL;DR

This study uses MHD simulations to analyze magnetic compression of FRCs, comparing results with 1D theory, revealing influences of initial conditions and ramping rates on FRC dynamics and validating theoretical predictions.

Contribution

The paper provides detailed MHD simulation analysis of FRC magnetic compression, exploring effects of initial profiles and magnetic ramping, and comparing results with existing 1D theoretical models.

Findings

Pressure evolution matches theoretical predictions.

FRC axial contraction depends on initial density and ramping rate.

FRC radius and density during compression are influenced by initial conditions and magnetic ramping.

Abstract

The magnetic compression has long been proposed a promising method for the plasma heating in a field reversed configuration (FRC), however, it remains a challenge to fully understand the physical mechanisms underlying the compression process, due to its highly dynamic nature beyond the one-dimensional (1D) adiabatic theory model [R. L. Spencer et al., Phys. Fluids 26, 1564 (1983)]. In this work, magnetohydrodynamics (MHD) simulations on the magnetic compression of FRCs using the NIMROD code [C. R. Sovinec et al., J. Comput. Phys. 195, 355 (2004)] and their comparisons with the 1D theory have been performed. The effects of the assumptions of the theory on the compression process have been explored, and the detailed profiles of the FRC during compression have been investigated. The pressure evolution agrees with the theoretical prediction under various initial conditions. The axial contraction of the FRC can be affected by the initial density profile and the ramping rate of the compression magnetic field, but the theoretical predictions on the FRC's length in general and the relation $r_s=\sqrt{2}r_o$ in particular hold approximately well during the whole compression process, where $r_s$ is the major radius of FRC separatrix and $r_o$ is that of the magnetic axis. The evolutions of the density and temperature can be affected significantly by the initial equilibrium profile and the ramping rate of the compression magnetic field. During the compression, the major radius of the FRC is another parameter that is susceptible to the ramping rate of the compression field. Basically, for the same magnetic compression ratio, the peak density is higher and the FRC's radius $r_s$ is smaller than the theoretical predictions.