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arxiv: 2008.06594 · v1 · pith:3QZGQ6FL · submitted 2020-08-14 · physics.plasm-ph · astro-ph.GA

Inefficient magnetic-field amplification in supersonic laser-plasma turbulence

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classification physics.plasm-ph astro-ph.GA
keywords magneticsupersonicfieldsinefficientlaser-plasmamoderatelyplasmaturbulence
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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 ($\mathrm{Rm} \approx 45$) 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.

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  1. The universal growth of magnetic energy during the nonlinear phase of subsonic and supersonic small-scale dynamos

    physics.plasm-ph 2025-09 unverdicted novelty 6.0

    Ensemble simulations find linear magnetic energy growth (p_nl=1) in subsonic small-scale dynamos and quadratic growth (p_nl=2) in supersonic ones, with universal conversion efficiency ~1/100 of turbulent kinetic energ...