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Laser-Produced Magnetic-Rayleigh-Taylor Unstable Plasma Slabs in a 20 T Magnetic Field

  • B. Khiar
  • , G. Revet
  • , A. Ciardi
  • , K. Burdonov
  • , E. Filippov
  • , J. Béard
  • , M. Cerchez
  • , S. N. Chen
  • , T. Gangolf
  • , S. S. Makarov
  • , M. Ouillé
  • , M. Safronova
  • , I. Yu Skobelev
  • , A. Soloviev
  • , M. Starodubtsev
  • , O. Willi
  • , S. Pikuz
  • , J. Fuchs
  • LERMA, Observatoire de Paris
  • Flash Center for Computational Science
  • Sorbonne Université
  • Institute of Applied Physics of the Russian Academy of Sciences
  • Joint Institute for High Temperatures of the Russian Academy of Sciences
  • CNRS
  • Heinrich Heine University Düsseldorf
  • Horia Hulubei National Institute of Physics and Nuclear Engineering
  • National Research Nuclear University MEPhI

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Magnetized laser-produced plasmas are central to many novel laboratory astrophysics and inertial confinement fusion studies, as well as in industrial applications. Here we provide the first complete description of the three-dimensional dynamics of a laser-driven plasma plume expanding in a 20 T transverse magnetic field. The plasma is collimated by the magnetic field into a slender, rapidly elongating slab, whose plasma-vacuum interface is unstable to the growth of the "classical," fluidlike magnetized Rayleigh-Taylor instability.

langue originaleAnglais
Numéro d'article205001
journalPhysical Review Letters
Volume123
Numéro de publication20
Les DOIs
étatPublié - 15 nov. 2019

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