Abstract
An experimental study of the magnetic field distribution in gas-puff pinches with and without a preembedded axial magnetic field () is presented. Spatially resolved, time-gated spectroscopic measurements were made at the Weizmann Institute of Science on a 300 kA, 1.6 μs rise time pulsed-power driver. The radial distribution of the azimuthal magnetic field, , during the implosion, with and without a preembedded axial magnetic field of , was measured using Zeeman polarization spectroscopy. The spectroscopic measurements of were consistent with the corresponding values of inferred from current measurements made with a B-dot probe. One-dimensional magnetohydrodynamic simulations, performed with the code trac-ii, showed agreement with the experimentally measured implosion trajectory, and qualitatively reproduced the experimentally measured radial profiles during the implosion when was applied. Simulation results of the radial profile of without a preembedded axial magnetic field did not qualitatively match experimental results due to magneto-Rayleigh-Taylor (MRT) instabilities. Our analysis emphasizes the importance of MRT instability mitigation when studying the magnetic field and current distributions in pinches. Discrepancies of the simulation results with experiment are discussed.
- Received 23 November 2020
- Accepted 5 April 2021
DOI:https://doi.org/10.1103/PhysRevE.103.053205
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