Passer à la navigation principale Passer à la recherche Passer au contenu principal

Inefficient Magnetic-Field Amplification in Supersonic Laser-Plasma Turbulence

  • A. F.A. Bott
  • , L. Chen
  • , G. Boutoux
  • , T. Caillaud
  • , A. Duval
  • , M. Koenig
  • , B. Khiar
  • , I. Lantuéjoul
  • , L. Le-Deroff
  • , B. Reville
  • , R. Rosch
  • , D. Ryu
  • , C. Spindloe
  • , B. Vauzour
  • , B. Villette
  • , A. A. Schekochihin
  • , D. Q. Lamb
  • , P. Tzeferacos
  • , G. Gregori
  • , A. Casner
  • University of Oxford
  • Princeton University
  • CEA/DAM
  • Osaka University
  • University of Chicago
  • CEA/UVSQ/CNRS
  • Max-Planck-Institut für Kernphysik
  • Ulsan National Institute of Science and Technology
  • Central Laser Facility
  • Merton College
  • University of Rochester
  • University of Rochester Laboratory for Laser Energetics
  • Univ. Bordeaux

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We report a laser-plasma experiment that was carried out at the LMJ-PETAL facility and realized the first magnetized, turbulent, supersonic () plasma with a large magnetic Reynolds number () in the laboratory. Initial seed magnetic fields were amplified, but only moderately so, and did not become dynamically significant. A notable absence of magnetic energy at scales smaller than the outer scale of the turbulent cascade was also observed. Our results support the notion that moderately supersonic, low-magnetic-Prandtl-number plasma turbulence is inefficient at amplifying magnetic fields compared to its subsonic, incompressible counterpart.

langue originaleAnglais
Numéro d'article175002
journalPhysical Review Letters
Volume127
Numéro de publication17
Les DOIs
étatPublié - 22 oct. 2021

Empreinte digitale

Examiner les sujets de recherche de « Inefficient Magnetic-Field Amplification in Supersonic Laser-Plasma Turbulence ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation