Onedimensional radiationhydrodynamic simulations of imploding spherical plasma liners with detailed equationofstate modeling
Abstract
This work extends the onedimensional radiationhydrodynamic imploding spherical argon plasma liner simulations of Awe et al.[Phys. Plasmas 18, 072705 (2011)] by using a detailed tabular equationofstate (EOS) model, whereas Awe et al. used a polytropic EOS model. Results using the tabular EOS model give lower stagnation pressures by a factor of 3.98.6 and lower peak ion temperatures compared to the polytropic EOS results. Both local thermodynamic equilibrium (LTE) and nonLTE EOS models were used in this work, giving similar results on stagnation pressure. The lower stagnation pressures using a tabular EOS model are attributed to a reduction in the liner's ability to compress arising from the energy sink introduced by ionization and electron excitation, which are not accounted for in a polytropic EOS model. Variation of the plasma liner species for the same initial liner geometry, mass density, and velocity was also explored using the LTE tabular EOS model, showing that the highest stagnation pressure is achieved with the highest atomic mass species for the constraints imposed.
 Authors:
 Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)
 Prism Computational Sciences, Inc., Madison, Wisconsin 53711 (United States)
 Propulsion Research Center, University of Alabama in Huntsville, Huntsville, Alabama 35899 (United States)
 Publication Date:
 OSTI Identifier:
 22068826
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Physics of Plasmas; Journal Volume: 19; Journal Issue: 10; Other Information: (c) 2012 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; ARGON; DENSITY; ELECTRONS; EQUATIONS OF STATE; EXCITATION; ION TEMPERATURE; LTE; MAGNETOHYDRODYNAMICS; ONEDIMENSIONAL CALCULATIONS; PLASMA; PLASMA SIMULATION; SPHERICAL CONFIGURATION; STAGNATION; THERMODYNAMICS
Citation Formats
Davis, J. S., Hsu, S. C., Golovkin, I. E., MacFarlane, J. J., and Cassibry, J. T.. Onedimensional radiationhydrodynamic simulations of imploding spherical plasma liners with detailed equationofstate modeling. United States: N. p., 2012.
Web. doi:10.1063/1.4757980.
Davis, J. S., Hsu, S. C., Golovkin, I. E., MacFarlane, J. J., & Cassibry, J. T.. Onedimensional radiationhydrodynamic simulations of imploding spherical plasma liners with detailed equationofstate modeling. United States. doi:10.1063/1.4757980.
Davis, J. S., Hsu, S. C., Golovkin, I. E., MacFarlane, J. J., and Cassibry, J. T.. 2012.
"Onedimensional radiationhydrodynamic simulations of imploding spherical plasma liners with detailed equationofstate modeling". United States.
doi:10.1063/1.4757980.
@article{osti_22068826,
title = {Onedimensional radiationhydrodynamic simulations of imploding spherical plasma liners with detailed equationofstate modeling},
author = {Davis, J. S. and Hsu, S. C. and Golovkin, I. E. and MacFarlane, J. J. and Cassibry, J. T.},
abstractNote = {This work extends the onedimensional radiationhydrodynamic imploding spherical argon plasma liner simulations of Awe et al.[Phys. Plasmas 18, 072705 (2011)] by using a detailed tabular equationofstate (EOS) model, whereas Awe et al. used a polytropic EOS model. Results using the tabular EOS model give lower stagnation pressures by a factor of 3.98.6 and lower peak ion temperatures compared to the polytropic EOS results. Both local thermodynamic equilibrium (LTE) and nonLTE EOS models were used in this work, giving similar results on stagnation pressure. The lower stagnation pressures using a tabular EOS model are attributed to a reduction in the liner's ability to compress arising from the energy sink introduced by ionization and electron excitation, which are not accounted for in a polytropic EOS model. Variation of the plasma liner species for the same initial liner geometry, mass density, and velocity was also explored using the LTE tabular EOS model, showing that the highest stagnation pressure is achieved with the highest atomic mass species for the constraints imposed.},
doi = {10.1063/1.4757980},
journal = {Physics of Plasmas},
number = 10,
volume = 19,
place = {United States},
year = 2012,
month =
}

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