Cross-code verification and sensitivity analysis to effectively model the electrothermal instability

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS High Energy Density Physics Pub Date : 2021-03-01 DOI:10.1016/j.hedp.2021.100925
R.L. Masti , C.L. Ellison , J.R. King , P.H. Stoltz , B. Srinivasan
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引用次数: 4

Abstract

This manuscript presents verification cases that are developed to study the electrothermal instability (ETI). Specific verification cases are included to ensure that the unit physics components necessary to model the ETI are accurate, providing a path for fluid-based codes to effectively simulate ETI in the linear and nonlinear growth regimes. Two software frameworks with different algorithmic approaches are compared for accuracy in their ability to simulate diffusion of a magnetic field, linear growth of the ETI, and a fully nonlinear ETI evolution. The nonlinear ETI simulations show early time agreement, with some differences emerging, as noted in the wavenumber spectrum, late into the nonlinear development of ETI. A sensitivity study explores the role of equation-of-state (EOS), vacuum density, and vacuum resistivity. EOS and vacuum resistivity are found to be the most critical factors in the modeling of nonlinear ETI development.

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交叉代码验证和灵敏度分析,有效地模拟了电热不稳定性
本文提出了用于研究电热不稳定性(ETI)的验证案例。包括具体的验证案例,以确保模拟ETI所需的单元物理组件是准确的,为基于流体的代码提供了一条路径,以有效地模拟线性和非线性增长体制下的ETI。比较了两种具有不同算法方法的软件框架在模拟磁场扩散、ETI线性增长和完全非线性ETI演化方面的准确性。非线性ETI模拟在早期时间上是一致的,但在ETI非线性发展的后期,出现了一些差异,如波数谱所示。灵敏度研究探讨了状态方程(EOS)、真空密度和真空电阻率的作用。发现EOS和真空电阻率是非线性ETI发展建模中最关键的因素。
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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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