Propagation of laser-generated plasma jet in an ambient medium

被引:7
|
作者
Loupias, B. [1 ]
Falize, E. [1 ]
Gregory, C. D. [2 ]
Vinci, T. [1 ,2 ]
Pikuz, S. [3 ]
Waugh, J. [4 ]
Koenig, M. [2 ]
Ravasio, A. [2 ]
Nazarov, W. [5 ]
Michaut, C. [6 ]
Bouquet, S. [1 ,6 ]
Kuramitsu, Y. [7 ]
Seiichi, D. [7 ]
Woolsey, N. C. [4 ]
Sakawa, Y. [7 ]
Takabe, H. [7 ]
Schiavi, A. [8 ,9 ]
Atzeni, S. [8 ,9 ]
机构
[1] CEA, DAM, DIF, F-91297 Arpajon, France
[2] Ecole Polytech, LULI, CNRS, CEA,UPMC, F-91128 Palaiseau, France
[3] RAS, Joint Inst High Temperatures, Moscow 125412, Russia
[4] Univ York, Dept Phys, York YO10 5DD, N Yorkshire, England
[5] Univ St Andrews, Sch Chem, St Andrews KY16 9ST, Fife, Scotland
[6] Univ Paris Diderot, LUTH, Observ Paris, CNRS, F-92190 Meudon, France
[7] Osaka Univ, Inst Laser Engn, Suita, Osaka 5650871, Japan
[8] Univ Roma La Sapienza, Dipartimento Energet, Rome, Italy
[9] CNISM, Rome, Italy
关键词
PROPER MOTIONS; BOW SHOCK; ASTROPHYSICS;
D O I
10.1088/0741-3335/51/12/124027
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 work we present experimental research related to laboratory astrophysics using an intense laser. The goal of these experiments is to investigate some of the complex features of young stellar objects and astrophysical outflows, in particular the plasma jet interaction with the interstellar medium. The relevance of these experiments to astrophysics is measured through similarity criteria (scaling laws). These ensure the similarity between the astrophysical object and the laboratory provided that the dimensionless numbers are equivalent. Consequently, measurements of the plasma parameters are crucial to link laboratory research to astrophysics as they are needed for the determination of these dimensionless numbers. In this context, we designed experiments to generate plasma jets using an intense laser, and to study the evolution in vacuum and in an ambient medium.
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页数:9
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