Formation and propagation of laser-driven plasma jets in an ambient medium studied with X-ray radiography and optical diagnostics

被引：8
|
作者：
Diziere, A. [1 ]
Pelka, A. [1 ]
Ravasio, A. [1 ]
Loupias, B. [2 ]
Falize, E. [2 ]
Kuramitsu, Y. [3 ]
Sakawa, Y. [3 ]
Morita, T. [3 ]
Pikuz, S. [4 ]
Yurchak, R. [1 ]
Koenig, M. [1 ,5 ]
机构：
[1] Ecole Polytech, CNRS, CEA, LULI,UPMC, Route Saclay, F-91128 Palaiseau, France
[2] DIF, CEA, DAM, F-91297 Arpajon, France
[3] Osaka Univ, Inst Laser Engn, Suita, Osaka 5650871, Japan
[4] RAS, Joint Inst High Temp, Moscow 125412, Russia
[5] Osaka Univ, Inst Acad Initiat, Suita, Osaka 5650871, Japan
来源：
PHYSICS OF PLASMAS | 2015年 / 22卷 / 01期
基金：
日本学术振兴会;
关键词：
SCALING LAWS; BOW SHOCK; FLOWS;
D O I：
10.1063/1.4905525
中图分类号：
O35 [流体力学]; O53 [等离子体物理学];
学科分类号：
070204 ; 080103 ; 080704 ;
摘要：
In this paper, we present experimental results obtained on the LULI2000 laser facility regarding structure and dynamics of astrophysical jets propagating in interstellar medium. The jets, generated by using a cone-shaped target, propagate in a nitrogen gas that mimics the interstellar medium. X-ray radiography as well as optical diagnostics were used to probe both high and low density regions. In this paper, we show how collimation of the jets evolves with the gas density. (C) 2015 AIP Publishing LLC.
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收藏
页数：6
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