期刊
HIGH ENERGY DENSITY PHYSICS
卷 22, 期 -, 页码 27-36出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.hedp.2017.01.005
关键词
-
资金
- Engineering and Physical Sciences Research Council [EP/K028464/1, EP/L000237/1]
- AWE Aldermaston
- EPSRC [EP/K028464/1, EP/L000237/1] Funding Source: UKRI
- Engineering and Physical Sciences Research Council [EP/K028464/1, 1102894, EP/L000237/1] Funding Source: researchfish
The Magnetized Liner Inertial Fusion (MagLIF) concept involves the compression of a magnetized fuel such that the stagnated fuel contains a magnetic field that can suppress heat flow losses and confine a particles. Magnetic confinement of a particles reduces the fuel rho R required for ignition. Recent work [1,2] has demonstrated that the magnitude of the magnetic field in deuterium fuel can be inferred from the yields and spectra of secondary DT neutrons. In this work we investigate the potential for using the shape of the secondary neutron spectra to diagnose the magnetic field topology in the stagnated fuel. Three different field topologies that could possibly occur in MagLIF experiments are studied: (1) a cylindrical fuel column containing axial and azimuthal magnetic field components, (2) a fuel column which is pinched at the ends to form a magnetic mirror and (3) a fuel column that has a helical tube shape with magnetic field lines following the helical path of the tube's axis. Each topology is motivated by observations from experimental or simulated MagLIF data. For each topology we use a multi-physics model to investigate the shapes of the secondary neutron spectra emitted from a steady-state stagnated fuel column. It is found that the azimuthal and helical topologies are more suitable than the mirror topology for reproducing an asymmetry in the axial spectra that was observed in experiments. Gorgon MHD simulations of the MagLIF implosion in 1D are also carried out. These show that sufficient azimuthal magnetic field can penetrate from the liner into the fuel to qualitatively reproduce the observed spectral asymmetry. (C) 2017 Elsevier B.V. All rights reserved.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据