| Literature DB >> 31809120 |
B Khiar1,2, G Revet3,4, A Ciardi1, K Burdonov1,3,4, E Filippov4,5, J Béard6, M Cerchez7, S N Chen8, T Gangolf3,7, S S Makarov5, M Ouillé3, M Safronova3,4, I Yu Skobelev5,9, A Soloviev4, M Starodubtsev4, O Willi7, S Pikuz5,9, J Fuchs3,4.
Abstract
Magnetized laser-produced plasmas are central to many novel laboratory astrophysics and inertial confinement fusion studies, as well as in industrial applications. Here we provide the first complete description of the three-dimensional dynamics of a laser-driven plasma plume expanding in a 20 T transverse magnetic field. The plasma is collimated by the magnetic field into a slender, rapidly elongating slab, whose plasma-vacuum interface is unstable to the growth of the "classical," fluidlike magnetized Rayleigh-Taylor instability.Year: 2019 PMID: 31809120 DOI: 10.1103/PhysRevLett.123.205001
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161