MHD Modeling of Plasma Generation and Radiation Transport Driven by the MG Field at the Metallic Surface

A. Esaulov, B. Bauer, R. Siemon, V. Makhin, S. Fuelling, T. Awe, R. Presura
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Abstract

Summary form only given. Recent experimental campaign at 1 MA (120 ns current rise time) Zebra pulse power generator reveals quite interesting dynamic picture of plasma production and evolution at the surface of the cylindrical metallic rods. Different rod diameters and rod materials have been explored. Multi-type plasma diagnostics included magnetic field probes, laser shadowgraphy, photodiodes, streak camera imaging etc. Radiation MHD modeling of plasma generation and evolution helps to interpret the experimental data and reveal additional features of plasma dynamics, hidden from direct experimental observations. Simulations have been performed with the Eulerian radiation and resistive two-temperature MHD code POS, modified to include both optically thin and optically thick plasma models into a single simulation. Radiation MHD modeling shows the generation of relatively hot and low-dense plasma fraction (that can be referred to as "corona") adjacent to the metallic surface, while the bulk of in plasma the metallic rod (or the "core") remains relatively cold, maintaining approximately the same mass density. Parameters of the coronal plasma depend on the road diameter and material used. This core-corona structure resembles the structure of the exploding wire. Simulations show that the coronal fraction of plasma is the main radiation emission source, while the intense radiation cooling keeps its temperature below 20 eV and prevents corona from further expansion after 80 ns. The intensity of the radiation transport in plasma has been compared against the kinetic transport effects, such as electron and ion thermal conductivities. Radiation post-processor of the radiation MHD code POS is used to resolve the radiation intensity versus the radiation wavelength and to rearrange the simulations data in the formats convenient for the direct comparison with such experimental data as the photodiode signals and streak-camera and laser shadowgraphy images.
金属表面MG场驱动等离子体产生和辐射输运的MHD模拟
只提供摘要形式。最近在1ma (120ns电流上升时间)斑马脉冲发电机上进行的实验揭示了圆柱形金属棒表面等离子体产生和演化的有趣动态图像。探索了不同的杆径和杆材。多类型等离子体诊断包括磁场探针、激光阴影成像、光电二极管、条纹相机成像等。等离子体产生和演化的辐射MHD模型有助于解释实验数据并揭示等离子体动力学的其他特征,这些特征隐藏在直接的实验观测中。用欧拉辐射和电阻双温MHD代码POS进行了模拟,修改后将光薄和光厚等离子体模型纳入单个模拟中。辐射MHD模型显示,在金属表面附近产生了相对热和低密度的等离子体部分(可称为“日冕”),而等离子体中的金属棒(或“核心”)仍然相对冷,保持大约相同的质量密度。日冕等离子体的参数取决于所使用的道路直径和材料。这种核心-电晕结构类似于爆炸电线的结构。模拟结果表明,等离子体的日冕部分是主要的辐射发射源,而强烈的辐射冷却使其温度低于20 eV,并阻止了80 ns后日冕的进一步膨胀。将等离子体中的辐射输运强度与电子和离子热传导等动力学输运效应进行了比较。利用辐射MHD码POS的辐射后置处理器解析辐射强度与辐射波长的关系,并将模拟数据重新整理成便于与光电二极管信号、条纹相机和激光阴影成像等实验数据直接比较的格式。
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