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Three-dimensional modeling of a plasma in a strong azimuthal magnetic field
Abstract
Three-dimensional magnetohydrodynamic (MHD) simulations are able to model the generation of disc-shaped plasma, driven by laser ablation from a current carrying rod in a pulsed-power machine producing azimuthal magnetic fields of 2–3 MG. The plasma at such extreme conditions is unique in that the parameter space for the plasma β and Hall parameter χ transition from below unity to greater than unity at different stages of the plasma generation. In simulations, the formation of the plasma disc in the azimuthal direction, is driven by heat flux from the laser spot and depends on the set of transport coefficients used in simulations. The most recent set of transport coefficients leads to the formation of plasma ejecta at the back end of the rod, that qualitatively matches experiments. Specifically, the cross-gradient Nernst effect, which twists magnetic field, is shown to have a large effect on the shape of the back end ejecta. In the direction along the axis of the rod there is propagation of perturbations from the disc as observed in experiments. In simulations the period of temperature perturbations is in good agreement with experimental results. Furthermore, an instability due to coupling of heat flux and the magnetic field advection providesmore »
- Authors:
-
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- University of Rochester, NY (United States)
- University of Nevada, Reno, NV (United States)
- Publication Date:
- Research Org.:
- Univ. of Rochester, NY (United States)
- Sponsoring Org.:
- USDOE; National Science Foundation (NSF)
- OSTI Identifier:
- 2320236
- Grant/Contract Number:
- NA0003856; AC52-07NA27344; PHY-1903355
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. E
- Additional Journal Information:
- Journal Volume: 109; Journal Issue: 1; Journal ID: ISSN 2470-0045
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; Laser-plasma interactions; Magnetohydrodynamics; Plasma instabilities; Plasma transport; Magnetized plasma; First-principles calculations in plasma physics; Imaging & optical processing; Magnetohydrodynamic techniques; Two-fluid & multi-fluid model
Citation Formats
Leal, Luis, Maximov, Andrei, García-Rubio, Fernando, Betti, Riccardo, and Ivanov, Vladimir. Three-dimensional modeling of a plasma in a strong azimuthal magnetic field. United States: N. p., 2024.
Web. doi:10.1103/physreve.109.015207.
Leal, Luis, Maximov, Andrei, García-Rubio, Fernando, Betti, Riccardo, & Ivanov, Vladimir. Three-dimensional modeling of a plasma in a strong azimuthal magnetic field. United States. https://doi.org/10.1103/physreve.109.015207
Leal, Luis, Maximov, Andrei, García-Rubio, Fernando, Betti, Riccardo, and Ivanov, Vladimir. Wed .
"Three-dimensional modeling of a plasma in a strong azimuthal magnetic field". United States. https://doi.org/10.1103/physreve.109.015207.
@article{osti_2320236,
title = {Three-dimensional modeling of a plasma in a strong azimuthal magnetic field},
author = {Leal, Luis and Maximov, Andrei and García-Rubio, Fernando and Betti, Riccardo and Ivanov, Vladimir},
abstractNote = {Three-dimensional magnetohydrodynamic (MHD) simulations are able to model the generation of disc-shaped plasma, driven by laser ablation from a current carrying rod in a pulsed-power machine producing azimuthal magnetic fields of 2–3 MG. The plasma at such extreme conditions is unique in that the parameter space for the plasma β and Hall parameter χ transition from below unity to greater than unity at different stages of the plasma generation. In simulations, the formation of the plasma disc in the azimuthal direction, is driven by heat flux from the laser spot and depends on the set of transport coefficients used in simulations. The most recent set of transport coefficients leads to the formation of plasma ejecta at the back end of the rod, that qualitatively matches experiments. Specifically, the cross-gradient Nernst effect, which twists magnetic field, is shown to have a large effect on the shape of the back end ejecta. In the direction along the axis of the rod there is propagation of perturbations from the disc as observed in experiments. In simulations the period of temperature perturbations is in good agreement with experimental results. Furthermore, an instability due to coupling of heat flux and the magnetic field advection provides a possible explanation for perturbation growth along the axis of the rod, and the instability growth rate is consistent with experimental results.},
doi = {10.1103/physreve.109.015207},
journal = {Physical Review. E},
number = 1,
volume = 109,
place = {United States},
year = {Wed Jan 24 00:00:00 EST 2024},
month = {Wed Jan 24 00:00:00 EST 2024}
}
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