Seeded Magneto Rayleigh-Taylor instability driven by a 1-MA Linear Transformer Driver

D. Chalenski, R. Gilgenbach, Y. Lau, Sonal G. Patel, A. Steiner, David Yager-Eliorraga, I. Rittersdorf, M. Weiss, M. Franzi, Peng Zhang, J. Zier
{"title":"Seeded Magneto Rayleigh-Taylor instability driven by a 1-MA Linear Transformer Driver","authors":"D. Chalenski, R. Gilgenbach, Y. Lau, Sonal G. Patel, A. Steiner, David Yager-Eliorraga, I. Rittersdorf, M. Weiss, M. Franzi, Peng Zhang, J. Zier","doi":"10.1109/MEGAGAUSS.2012.6781453","DOIUrl":null,"url":null,"abstract":"Experimental, theoretical and simulation research investigations are underway on the Magneto Rayleigh-Taylor instability driven by the Mega Ampere Linear Transformer Driver at the University of Michigan. Since the Linear Transformer Driver operates at 100- kV output, inductance minimization was crucial in design of the coaxial and radial magnetically insulated transmission line that transmits power to the load. Experiments ablate a 400 nm-thick, 1 cm wide, planar, aluminum foil located between two parallel-plate anodes. The initial position of the foil relative to the anodes controls the foil-plasma acceleration. Laser-micromachined, periodic hole patterns on foils are utilized to seed the wavelength of Magneto Rayleigh-Taylor growth. Sub-ns laser shadowgraphy diagnoses the instability growth at the edges of the ablation plasma. Early instability is believed to originate from the Electro-Thermal instability. Later exponential growth rates have been measured whose trends are consistent with Magneto Rayleigh Taylor theory. As expected, the fastest Magneto Rayleigh-Taylor growth rate corresponds to the largest foil-plasma acceleration. Effects of magnetic shear on Magneto Rayleigh-Taylor growth have been predicted theoretically.","PeriodicalId":299352,"journal":{"name":"2012 14th International Conference on Megagauss Magnetic Field Generation and Related Topics (MEGAGAUSS)","volume":"126 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2012-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"2012 14th International Conference on Megagauss Magnetic Field Generation and Related Topics (MEGAGAUSS)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/MEGAGAUSS.2012.6781453","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

Experimental, theoretical and simulation research investigations are underway on the Magneto Rayleigh-Taylor instability driven by the Mega Ampere Linear Transformer Driver at the University of Michigan. Since the Linear Transformer Driver operates at 100- kV output, inductance minimization was crucial in design of the coaxial and radial magnetically insulated transmission line that transmits power to the load. Experiments ablate a 400 nm-thick, 1 cm wide, planar, aluminum foil located between two parallel-plate anodes. The initial position of the foil relative to the anodes controls the foil-plasma acceleration. Laser-micromachined, periodic hole patterns on foils are utilized to seed the wavelength of Magneto Rayleigh-Taylor growth. Sub-ns laser shadowgraphy diagnoses the instability growth at the edges of the ablation plasma. Early instability is believed to originate from the Electro-Thermal instability. Later exponential growth rates have been measured whose trends are consistent with Magneto Rayleigh Taylor theory. As expected, the fastest Magneto Rayleigh-Taylor growth rate corresponds to the largest foil-plasma acceleration. Effects of magnetic shear on Magneto Rayleigh-Taylor growth have been predicted theoretically.
由1毫安线性变压器驱动器驱动的种子磁瑞利-泰勒不稳定性
密歇根大学正在进行实验、理论和模拟研究,研究由百万安培线性变压器驱动器驱动的磁瑞利-泰勒不稳定性。由于线性变压器驱动器工作在100千伏输出,电感最小化在同轴和径向磁绝缘传输线的设计是至关重要的,向负载传输电力。实验烧蚀一块400纳米厚,1厘米宽的平面铝箔,位于两个平行板阳极之间。箔片相对于阳极的初始位置控制箔片等离子体加速度。利用激光微机械加工,在箔上的周期性孔图案来播种磁瑞利-泰勒生长的波长。亚毫米波激光阴影成像诊断烧蚀等离子体边缘的不稳定生长。早期不稳定性被认为是由电-热不稳定性引起的。后来测量的指数增长率的趋势与万磁王瑞利·泰勒理论相一致。正如预期的那样,最快的磁瑞利-泰勒增长率对应于最大的箔等离子体加速度。从理论上预测了磁剪切对磁瑞利-泰勒生长的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信