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

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Article number175002
JournalPhysical Review Letters
Volume127
Issue number17
DOIs
Publication statusPublished - 22 Oct 2021

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