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Two-dimensional MHD simulations of a neon Z pinch on Hawk
被引:4
|作者:
Schumer, JW
[1
]
Mosher, D
Moosman, B
Weber, BV
Commisso, RJ
Qi, NS
Schein, J
Krishnan, M
机构:
[1] USN, Res Lab, Div Plasma Phys, Washington, DC 20375 USA
[2] Alameda Appl Sci Corp, San Leandro, CA 94577 USA
关键词:
MHD simulations;
neon gas puff;
plasma radiation source;
snow-plow implosions;
Z pinch;
D O I:
10.1109/TPS.2002.1024281
中图分类号:
O35 [流体力学];
O53 [等离子体物理学];
学科分类号:
070204 ;
080103 ;
080704 ;
摘要:
Two-dimensional magnetohydrodynamic (MHD) simulations using MACH2 are benchmarked against laser shearing interferometer (LSI) images of the evolving electron-density sheath during 250-ns neon gas-puff z pinch implosions on the Naval Research Laboratory Hawk generator. The initial density distribution for the MHD simulations is calculated using a ballistic-flow-model fit to the measured initial gas-density distributions. The implosion is modeled using an applied current profile, single-temperature energy equations, and black-body-limited optically thin radiation. For consistency with the radiation model, neon ionization and equation-of-state models have been added to MACH2. Computed MHD ion-density distributions compare well with LSI images as the snowplowed plasma channel evolves during implosion. The MHD results also show features that may be helpful for understanding early and weak K-shell radiation observed near the nozzle in Double-Eagle gas-puff experiments. Current-channel evolution derived from one-dimensional snow-plow calculations compare well to the MHD results for the same current history and initial density distribution, indicating that axial mass flow does not strongly impact the implosion dynamics.
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页码:488 / 497
页数:10
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