Characterization of the stability and dynamics of a laser-produced plasma expanding across a strong magnetic field

被引:6
|
作者
Yao, Weipeng [1 ,2 ]
Capitaine, Julien [2 ]
Khiar, Benjamin [3 ]
Vinci, Tommaso [1 ]
Burdonov, Konstantin [1 ,2 ,4 ]
Beard, Jerome [5 ]
Fuchs, Julien [1 ]
Ciardi, Andrea [2 ]
机构
[1] Sorbonne Univ, Ecole Polytech, Inst Polytech Paris, LULI CNRS,CEA, F-91128 Palaiseau, France
[2] Univ PSL, Sorbonne Univ, Observ Paris, CNRS,LERMA, F-75005 Paris, France
[3] Off Natl Etud & Rech Aerosp ONERA, F-91123 Palaiseau, France
[4] Russian Acad Sci, IAP, Nizhnii Novgorod 603950, Russia
[5] CNRS UGA UPS INSA, UPR 3228, LNCMI, F-31400 Toulouse, France
基金
欧洲研究理事会;
关键词
INSTABILITY; SIMULATION; JETS;
D O I
10.1063/5.0058306
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Magnetized laser-produced plasmas are central to many studies in laboratory astrophysics, in inertial confinement fusion, and in industrial applications. Here, we present the results of large-scale three-dimensional magnetohydrodynamic simulations of the dynamics of a laser-produced plasma expanding into a transverse magnetic field with a strength of tens of teslas. The simulations show the plasma being confined by the strong magnetic field into a slender slab structured by the magnetized Rayleigh-Taylor instability that develops at the plasma-vacuum interface. We find that when the initial velocity of the plume is perturbed, the slab can develop kink-like motions that disrupt its propagation. (c) 2022 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
引用
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页数:9
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