TY - JOUR
T1 - Micron-scale phenomena observed in a turbulent laser-produced plasma
AU - Rigon, G.
AU - Albertazzi, B.
AU - Pikuz, T.
AU - Mabey, P.
AU - Bouffetier, V.
AU - Ozaki, N.
AU - Vinci, T.
AU - Barbato, F.
AU - Falize, E.
AU - Inubushi, Y.
AU - Kamimura, N.
AU - Katagiri, K.
AU - Makarov, S.
AU - Manuel, M. J.E.
AU - Miyanishi, K.
AU - Pikuz, S.
AU - Poujade, O.
AU - Sueda, K.
AU - Togashi, T.
AU - Umeda, Y.
AU - Yabashi, M.
AU - Yabuuchi, T.
AU - Gregori, G.
AU - Kodama, R.
AU - Casner, A.
AU - Koenig, M.
N1 - Publisher Copyright:
© 2021, The Author(s).
PY - 2021/12/1
Y1 - 2021/12/1
N2 - 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 (~1μm) over a large field of view (>1 mm2). 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.
AB - 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 (~1μm) over a large field of view (>1 mm2). 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.
UR - https://www.scopus.com/pages/publications/85105771855
U2 - 10.1038/s41467-021-22891-w
DO - 10.1038/s41467-021-22891-w
M3 - Article
C2 - 33976145
AN - SCOPUS:85105771855
SN - 2041-1723
VL - 12
JO - Nature Communications
JF - Nature Communications
IS - 1
M1 - 2679
ER -