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Shock formation in Ne, Ar, Kr, and Xe on deuterium gas puff implosions
Author(s) -
J. Narkis,
H. U. Rahman,
P. Ney,
M. P. Desjarlais,
F. J. Wessel,
F. Conti,
J. C. Valenzuela,
F. N. Beg
Publication year - 2016
Publication title -
physics of plasmas
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.75
H-Index - 160
eISSN - 1089-7674
pISSN - 1070-664X
DOI - 10.1063/1.4972547
Subject(s) - physics , atomic physics , adiabatic process , shock (circulatory) , implosion , plasma , shock wave , magnetohydrodynamics , rayleigh–taylor instability , instability , z pinch , radius , compression (physics) , mechanics , nuclear physics , thermodynamics , medicine , computer security , computer science
1- and 2-D simulations of 1-cm radius, gas-puff liners of Ne, Ar, Kr, and Xe imploding onto a deuterium target are conducted using the discharge parameters for the Zebra (1 MA, 130 ns) driver using the resistive MHD code MACH2. This is an implementation of the Staged Z-pinch concept, in which the target is driven to high-energy-density first by shock compression launched by a diffused azimuthal magnetic field ( J×B force), and then by the adiabatic compression as the liner converges on axis. During the run-in phase, the initial shock heating preheats the deuterium plasma, with a subsequent stable, adiabatic compression heating the target to high energy density. Shock compression of the target coincides with the development of a J×B force at the target/liner interface. Stronger B-field transport and earlier shock compression increases with higher-Z liners, which results in an earlier shock arrival on axis. Delayed shock formation in lower-Z liners yields a relative increase in shock heating, however, the 2...

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