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.
引用
收藏
页码:488 / 497
页数:10
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