The Challenge of Wall-Plasma Interaction with Pulsed MG Fields Parallel to the Wall

R. Siemon, B. Bauer, T. Awe, M. Angelova, S. Fuelling, T. Goodrich, I. Lindemuth, V. Makhin, V. Ivanov, R. Presura, W. Atchison, R. Faehl, R. Reinovsky, D. Scudder, P. Turchi, J. Degnan, E. Ruden, M. Frese, S. Garanin, V. Mokhov
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引用次数: 5

Abstract

Experiments suitable for a variety of pulsed power facilities are being developed to study plasma formation and stability on the surface of typical liner materials in the megagauss (MG) regime. Understanding the plasma properties near the surface is likely to be critical for the design of Magnetized Target Fusion experiments, where the plasma density in the region near the wall can play an important role in setting the transport from hot fuel to the cold boundary. From the perspective of diagnostic access and simplicity, the surface of a stationary conductor with large enough current to generate MG surface field offers advantages compared with studying the surface of a moving liner. This paper reports on recent experiments at UNR that have generated magnetic fields in the range of about 0.2 to 3 MG, which confirm the viability of future experiments planned at Atlas and/or Shiva Star. Diagnostics reported here involve electrical measurements, streak camera photography, and surface luminosity. Additional diagnostic measurements and numerical modeling will be reported in the future.
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平行于壁的脉冲MG场对壁-等离子体相互作用的挑战
目前,人们正在开发适合各种脉冲功率设备的实验,以研究典型的百万高斯(MG)条件下衬里材料表面等离子体的形成和稳定性。了解表面附近的等离子体特性可能对磁化靶聚变实验的设计至关重要,其中壁面附近区域的等离子体密度在设置从热燃料到冷边界的输运中起着重要作用。从诊断的可及性和简单性的角度来看,具有足够大电流产生MG表面场的静止导体表面与研究运动衬垫表面相比具有优势。本文报告了联合国研究中心最近的实验,这些实验产生了约0.2至3毫克范围的磁场,这证实了计划在阿特拉斯和/或希瓦星进行的未来实验的可行性。这里报道的诊断包括电测量、条纹相机摄影和表面亮度。更多的诊断测量和数值模拟将在未来报道。
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