Inefficient magnetic-field amplification in supersonic laser-plasma turbulence
Plasma Physics
2021-11-03 v1 Astrophysics of Galaxies
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.
Keywords
Cite
@article{arxiv.2008.06594,
title = {Inefficient magnetic-field amplification in supersonic laser-plasma turbulence},
author = {A. F. A. Bott and L. Chen and G. Boutoux and T. Caillaud and A. Duval and M. Koenig and B. Khiar and I. Lantuéjoul and L. Le-Deroff and B. Reville and R. Rosch and D. Ryu and C. Spindloe and B. Vauzour and B. Villette and A. A. Schekochihin and D. Q. Lamb and P. Tzeferacos and G. Gregori and A. Casner},
journal= {arXiv preprint arXiv:2008.06594},
year = {2021}
}
Comments
6 pages, 4 figures; supplemental information included (14 pages, 10 figures)