Inefficient Magnetic-Field Amplification in Supersonic Laser-Plasma Turbulence.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
22 Oct 2021
Historique:
received: 20 08 2020
revised: 07 06 2021
accepted: 17 09 2021
entrez: 5 11 2021
pubmed: 6 11 2021
medline: 6 11 2021
Statut: ppublish

Résumé

We report a laser-plasma experiment that was carried out at the LMJ-PETAL facility and realized the first magnetized, turbulent, supersonic (Ma_{turb}≈2.5) plasma with a large magnetic Reynolds number (Rm≈45) 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.

Identifiants

pubmed: 34739267
doi: 10.1103/PhysRevLett.127.175002
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

175002

Auteurs

A F A Bott (AFA)

Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom.
Department of Astrophysical Sciences, University of Princeton, 4 Ivy Lane, Princeton, New Jersey 08544, USA.

L Chen (L)

Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom.

G Boutoux (G)

CEA-DAM, DIF, F-91297 Arpajon, France.

T Caillaud (T)

CEA-DAM, DIF, F-91297 Arpajon, France.

A Duval (A)

CEA-DAM, DIF, F-91297 Arpajon, France.

M Koenig (M)

LULI, CNRS, CEA, Ecole Polytechnique, UPMC, Sorbonne Universités, Institut Polytechnique de Paris, F-91128 Palaiseau cedex, France.
Graduate School of Engineering, Osaka University, Suita, Osaka 565-0871, Japan.

B Khiar (B)

Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Avenue, Chicago, Illinois 60637, USA.

I Lantuéjoul (I)

CEA-DAM, DIF, F-91297 Arpajon, France.

L Le-Deroff (L)

CEA, DAM, CESTA, F-33114 Le Barp, France.

B Reville (B)

Max-Planck-Institut für Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany.

R Rosch (R)

CEA-DAM, DIF, F-91297 Arpajon, France.

D Ryu (D)

Department of Physics, School of Natural Sciences, UNIST, Ulsan 44919, Korea.

C Spindloe (C)

Central Laser Facility, STFC Rutherford Appleton Laboratory, Chilton, Didcot OX11 0XQ, United Kingdom.

B Vauzour (B)

CEA-DAM, DIF, F-91297 Arpajon, France.

B Villette (B)

CEA-DAM, DIF, F-91297 Arpajon, France.

A A Schekochihin (AA)

Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom.
Merton College, Merton Street, Oxford OX1 4JD, United Kingdom.

D Q Lamb (DQ)

Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Avenue, Chicago, Illinois 60637, USA.

P Tzeferacos (P)

Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom.
Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Avenue, Chicago, Illinois 60637, USA.
Department of Physics and Astronomy, University of Rochester, 206 Bausch & Lomb Hall, Rochester, New York 14627, USA.
Laboratory for Laser Energetics, University of Rochester, 250 East River Road, Rochester, New York 14623, USA.

G Gregori (G)

Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom.

A Casner (A)

CEA-DAM, DIF, F-91297 Arpajon, France.
Université de Bordeaux-CNRS-CEA, CELIA, UMR 5107, F-33405 Talence, France.

Classifications MeSH