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

Authors :
Weipeng Yao
Julien Capitaine
Benjamin Khiar
Tommaso Vinci
Konstantin Burdonov
Jérôme Béard
Julien Fuchs
Andrea Ciardi
Laboratoire pour l'utilisation des lasers intenses (LULI)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
LERMA Cergy (LERMA)
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres (LERMA)
École normale supérieure - Paris (ENS-PSL)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)-École normale supérieure - Paris (ENS-PSL)
Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)
DPHY, ONERA, Université Paris Saclay [Palaiseau]
ONERA-Université Paris-Saclay
A.M.Obukhov Institute of Atmospheric Physics (IAP)
Russian Academy of Sciences [Moscow] (RAS)
Laboratoire national des champs magnétiques intenses - Toulouse (LNCMI-T)
Institut National des Sciences Appliquées - Toulouse (INSA Toulouse)
Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)
ANR-10-EQPX-0029,EQUIP@MESO,Equipement d'excellence de calcul intensif de Mesocentres coordonnés - Tremplin vers le calcul petaflopique et l'exascale(2010)
European Project: 787539,GENESIS - 10.3030/787539
Source :
Matter and Radiation at Extremes, Matter and Radiation at Extremes, 2022, 7, pp.026903. ⟨10.1063/5.0058306⟩, Matter and Radiation at Extremes, 2022, 7 (2), pp.026903. ⟨10.1063/5.0058306⟩
Publication Year :
2021

Abstract

International audience; Magnetized laser-produced plasmas are central to many new studies in laboratory astrophysics, inertial confinement fusion, and in industrial applications. Here we present the results of large-scale, three-dimensional magneto-hydrodynamic simulations of the dynamics of a laser-produced plasma expanding into a transverse magnetic field with strength of tens of Tesla. 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 by perturbing the initial velocity of the plume the slab can develops kink-like motion which disrupt its propagation, as observed in recent experiments.

Details

Language :
English
ISSN :
2468080X
Database :
OpenAIRE
Journal :
Matter and Radiation at Extremes, Matter and Radiation at Extremes, 2022, 7, pp.026903. ⟨10.1063/5.0058306⟩, Matter and Radiation at Extremes, 2022, 7 (2), pp.026903. ⟨10.1063/5.0058306⟩
Accession number :
edsair.doi.dedup.....b3622aee4ece605279bd490ef75fbc76