Modified helix-like instability structure on imploding z-pinch liners that are pre-imposed with a uniform axial magnetic field

被引:80
作者
Awe, T. J. [1 ]
Jennings, C. A. [1 ]
McBride, R. D. [1 ]
Cuneo, M. E. [1 ]
Lamppa, D. C. [1 ]
Martin, M. R. [1 ]
Rovang, D. C. [1 ]
Sinars, D. B. [1 ]
Slutz, S. A. [1 ]
Owen, A. C. [1 ]
Tomlinson, K. [2 ]
Gomez, M. R. [1 ]
Hansen, S. B. [1 ]
Herrmann, M. C. [1 ]
Jones, M. C. [1 ]
McKenney, J. L. [1 ]
Robertson, G. K. [1 ]
Rochau, G. A. [1 ]
Savage, M. E. [1 ]
Schroen, D. G. [2 ]
Stygar, W. A. [1 ]
机构
[1] Sandia Natl Labs, Albuquerque, NM 87185 USA
[2] Gen Atom Co, San Diego, CA 92121 USA
关键词
22;
D O I
10.1063/1.4872331
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
Recent experiments at the Sandia National Laboratories Z Facility have, for the first time, studied the implosion dynamics of magnetized liner inertial fusion (MagLIF) style liners that were pre-imposed with a uniform axial magnetic field. As reported [T. J. Awe et al., Phys. Rev. Lett. 111, 235005 (2013)] when premagnetized with a 7 or 10 T axial field, these liners developed 3D-helix-like hydrodynamic instabilities; such instabilities starkly contrast with the azimuthally correlated magneto-Rayleigh-Taylor (MRT) instabilities that have been consistently observed in many earlier non-premagnetized experiments. The helical structure persisted throughout the implosion, even though the azimuthal drive field greatly exceeded the expected axial field at the liner's outer wall for all but the earliest stages of the experiment. Whether this modified instability structure has practical importance for magneto-inertial fusion concepts depends primarily on whether the modified instability structure is more stable than standard azimuthally correlated MRT instabilities. In this manuscript, we discuss the evolution of the helix-like instability observed on premagnetized liners. While a first principles explanation of this observation remains elusive, recent 3D simulations suggest that if a small amplitude helical perturbation can be seeded on the liner's outer surface, no further influence from the axial field is required for the instability to grow. (C) 2014 AIP Publishing LLC.
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页数:8
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