Resistive diffusion in magnetized ICF implosions: Reduced magnetic stabilization of the Richtmyer–Meshkov instability

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
C.A. Walsh , D.J. Strozzi , H. Sio , B.B. Pollock , B.D. Appelbe , A.J. Crilly , S. O’Neill , C. Weber , J.P. Chittenden , J.D. Moody
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引用次数: 0

Abstract

Resistive diffusion is typically regarded to be negligible in magnetized ICF experiments, with magnetic flux effectively compressed during the implosion. In this work the Richtmyer–Meshkov instability at the ice-ablator interface is taken as an example for investigating resistive effects. For a high temperature (100eV) interface with magnetic field applied perpendicular to shock propagation, perturbation growth is suppressed by magnetic tension. However, for lower temperature interfaces the resistive diffusion prevents substantial magnetic field twisting at small scales. ICF implosion simulations are then used to assess magnetic diffusivity at different interfaces; the ice-ablator interface is found to be too resistive for the magnetic fields to enhance stability. For Rayleigh–Taylor growth at the hot-spot edge, on the other hand, resistivity is estimated to only be a secondary effect, as seen in previous simulation studies.

磁化 ICF 内爆中的电阻扩散:Richtmyer-Meshkov 不稳定性的减磁稳定性
在磁化 ICF 实验中,通常认为电阻扩散可以忽略不计,因为磁通量在内爆过程中会被有效压缩。在这项工作中,以冰-内爆器界面的里氏-梅什科夫不稳定性为例,研究了电阻效应。对于磁场垂直于冲击传播的高温(≈100eV)界面,磁张力抑制了扰动增长。然而,对于温度较低的界面,电阻扩散阻止了小尺度磁场的大幅扭曲。然后,利用 ICF 内爆模拟来评估不同界面的磁扩散性;结果发现,冰-冲击器界面的电阻性太强,磁场无法增强稳定性。另一方面,对于热点边缘的瑞利-泰勒(Rayleigh-Taylor)增长,电阻率估计只是次要影响,这一点在以前的模拟研究中已经看到。
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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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