4.8 Article

Micron-scale phenomena observed in a turbulent laser-produced plasma

Journal

NATURE COMMUNICATIONS
Volume 12, Issue 1, Pages -

Publisher

NATURE RESEARCH
DOI: 10.1038/s41467-021-22891-w

Keywords

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Funding

  1. Agence Nationale de la Recherche (ANR) [ANR-15-CE30-0011]
  2. Investissements d'Avenir from the LabEx PALM [ANR-10-LABX-0039-PALM]
  3. CNRS
  4. ANR [ANR-10-IDEX-03-02]
  5. KAKENHI from Japan Society for the Promotion of Science (JSPS) [16H02246, 17K05729]
  6. X-ray Free Electron Laser Priority Strategy Programme (Osaka University) [12005014]
  7. Quantum Leap Programme from the Ministry of Education, Culture, Sports, Science, and Technology (MEXT) [JPMXS0118067246, JPMXS0118070187]
  8. Ministry for Science and Higher Education of the Russian Federation [075-15-2020-785]
  9. Russian Foundation for Basic Research [19-32-90142]
  10. Engineering and Physical Sciences Research Council [EP/M022331/1, EP/N014472/1]
  11. Grants-in-Aid for Scientific Research [17K05729] Funding Source: KAKEN

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This study successfully measured the turbulent spectrum in a laser-plasma experiment at the micron scale, providing a platform for the direct comparison of experimental results, theory, and numerical simulations.
Turbulence is ubiquitous in the universe and in fluid dynamics. It influences a wide range of high energy density systems, from inertial confinement fusion to astrophysical-object evolution. Understanding this phenomenon is crucial, however, due to limitations in experimental and numerical methods in plasma systems, a complete description of the turbulent spectrum is still lacking. Here, we present the measurement of a turbulent spectrum down to micron scale in a laser-plasma experiment. We use an experimental platform, which couples a high power optical laser, an x-ray free-electron laser and a lithium fluoride crystal, to study the dynamics of a plasma flow with micrometric resolution (similar to 1 mu m) over a large field of view (>1 mm(2)). After the evolution of a Rayleigh-Taylor unstable system, we obtain spectra, which are overall consistent with existing turbulent theory, but present unexpected features. This work paves the way towards a better understanding of numerous systems, as it allows the direct comparison of experimental results, theory and numerical simulations.

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