Magnetic-field generation by the ablative nonlinear Rayleigh-Taylor instability

被引：4

作者：

Nilson, Philip M. ^{[1
,2
]}

Gao, L. ^{[1
,3
]}

Igumenshchev, I. V. ^{[1
]}

Fiksel, G. ^{[1
]}

Yan, R. ^{[1
,2
,3
]}

Davies, J. R. ^{[1
,2
,3
]}

Martinez, D. ^{[4
]}

Smalyuk, V. A. ^{[4
]}

Haines, M. G. ^{[5
]}

Blackman, E. G. ^{[1
,6
]}

Froula, D. H. ^{[1
]}

Betti, R. ^{[1
,2
,3
,6
]}

Meyerhofer, D. D. ^{[1
,2
,3
,6
]}

机构：

[1] Univ Rochester, Laser Energet Lab, Rochester, NY 14623 USA

[2] Univ Rochester, Fus Sci Ctr, Rochester, NY 14623 USA

[3] Univ Rochester, Dept Mech Engn, Rochester, NY 14623 USA

[4] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

[5] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London SW7 2AZ, England

[6] Univ Rochester, Dept Phys, Rochester, NY 14623 USA

来源：

JOURNAL OF PLASMA PHYSICS | 2015年 / 81卷

关键词：

INERTIAL CONFINEMENT FUSION; SCALING LAWS; OMEGA LASER;

D O I：

10.1017/S0022377814001093

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：

Experiments reporting magnetic-field generation by the ablative nonlinear Rayleigh-Taylor (RT) instability are reviewed. The experiments show how large-scale magnetic fields can, under certain circumstances, emerge and persist in strongly driven laboratory and astrophysical flows at drive pressures exceeding one million times atmospheric pressure.

引用

页数：12

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