Filippov Evgeny D, Makarov Sergey S, Burdonov Konstantin F, Yao Weipeng, Revet Guilhem, Béard Jerome, Bolaños Simon, Chen Sophia N, Guediche Amira, Hare Jack, Romanovsky Denis, Skobelev Igor Yu, Starodubtsev Mikhail, Ciardi Andrea, Pikuz Sergey A, Fuchs Julien
Institute of Applied Physics, RAS, 46 Ulyanov Street, Nizhny Novgorod, Russia, 603950.
Joint Institute for High Temperatures, RAS, 13 Bd.2 Izhorskaya st., Moscow, Russia, 125412.
Sci Rep. 2021 Apr 14;11(1):8180. doi: 10.1038/s41598-021-87651-8.
We analyze, using experiments and 3D MHD numerical simulations, the dynamic and radiative properties of a plasma ablated by a laser (1 ns, 10[Formula: see text]-10[Formula: see text] W/cm[Formula: see text]) from a solid target as it expands into a homogeneous, strong magnetic field (up to 30 T) that is transverse to its main expansion axis. We find that as early as 2 ns after the start of the expansion, the plasma becomes constrained by the magnetic field. As the magnetic field strength is increased, more plasma is confined close to the target and is heated by magnetic compression. We also observe that after [Formula: see text] ns, the plasma is being overall shaped in a slab, with the plasma being compressed perpendicularly to the magnetic field, and being extended along the magnetic field direction. This dense slab rapidly expands into vacuum; however, it contains only [Formula: see text] of the total plasma. As a result of the higher density and increased heating of the plasma confined against the laser-irradiated solid target, there is a net enhancement of the total X-ray emissivity induced by the magnetization.
我们通过实验和三维磁流体动力学数值模拟,分析了被激光(1纳秒,10[公式:见原文]-10[公式:见原文]瓦/平方厘米)从固体靶材烧蚀出的等离子体在向与其主膨胀轴垂直的均匀强磁场(高达30特斯拉)中膨胀时的动力学和辐射特性。我们发现,早在膨胀开始后2纳秒,等离子体就受到磁场的约束。随着磁场强度增加,更多等离子体被限制在靶材附近,并通过磁压缩被加热。我们还观察到,在[公式:见原文]纳秒后,等离子体整体呈平板状,等离子体在垂直于磁场方向被压缩,并沿磁场方向延伸。这个致密的平板迅速向真空中膨胀;然而,它仅包含总等离子体的[公式:见原文]。由于被限制在激光辐照固体靶材上的等离子体密度更高且加热增强,磁化诱导的总X射线发射率有净增强。