Collisionless plasma astrophysics simulation experiments using lasers

被引:0
|
作者
Woolsey, N. C. [1 ]
Ash, A. D. [1 ]
Courtois, C. [1 ]
Dendy, R. O. [2 ]
Gregory, C. D. [1 ]
Hall, I. M. [1 ]
Howe, J. [1 ]
机构
[1] Univ York, Dept Phys, York YO10 5DD, N Yorkshire, England
[2] AEA Technol, Culham Div, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
来源
基金
英国工程与自然科学研究理事会;
关键词
laser-produced-plasma; shocks; supemova remnants; strong magnetic fields;
D O I
暂无
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Laboratory experiment is an attractive method of exploring the plasma physics that may occur in solar and astrophysical shocks. An experiment enables repeated and detailed measurements of a plasma as the input conditions are adjusted. To form a scaled experiment of an astrophysical shock a plasma physics model of the shock is required, and the important dimensionless parameters identified and reproduced in the laboratory. A laboratory simulation of a young supernova remnant is described. The experiment uses the interaction of two millimetre-sized counter-streaming laser-produced plasmas placed in a strong transverse magnetic field to achieve this scaling. The collision-free dynamics of the two plasmas and their interaction are studied with and without the magnetic field through spatially and temporally resolved optical measurements. Laboratory astroplasma physics experiments using high-energy, high-power laser technology enables us to reproduce in the laboratory the conditions of temperature and pressure that are met in extreme stellar environments.
引用
收藏
页码:365 / +
页数:2
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