Studies of high energy density physics and laboratory astrophysics driven by intense lasers

被引：1
|
作者：
Zhang, J. [1 ,2 ,3 ]
Li, Y. T. [3 ,4 ]
Chen, L. M. [3 ,4 ]
Dong, Q. L. [3 ,5 ]
Zhong, J. Y. [3 ,6 ]
Wang, W. M. [3 ,4 ]
Sheng, Z. M. [1 ,2 ,3 ,7 ]
Zhao, G. [8 ]
机构：
[1] Shanghai Jiao Tong Univ, Minist Educ, Key Lab Laser Plasmas, Shanghai, Peoples R China
[2] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai, Peoples R China
[3] Shanghai Jiao Tong Univ, Collaborat Innovat Ctr Inertial Fus Sci & Applica, Shanghai, Peoples R China
[4] Chinese Acad Sci, Inst Phys, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China
[5] Ludong Univ, Sch Phys & Optoelect, Yantai 264025, Peoples R China
[6] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
[7] Univ Strathclyde, Dept Phys, SUPA, Glasgow, Lanark, Scotland
[8] Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China
来源：
9TH INTERNATIONAL CONFERENCE ON INERTIAL FUSION SCIENCES AND APPLICATIONS (IFSA 2015) | 2016年 / 717卷
关键词：
X-RAY SOURCE; MAGNETIC-FIELD; SOLAR-FLARE; ACCELERATION; GENERATION; PLASMA;
D O I：
10.1088/1742-6596/717/1/012004
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
Laser plasmas are capable of creating unique physical conditions with extreme high energy density, which are not only closely relevant to inertial fusion energy studies, but also to laboratory simulation of some astrophysical processes. In this paper, we highlight some recent progress made by our research teams. The first part is about directional hot electron beam generation and transport for fast ignition of inertial confinement fusion, as well as a new scheme of fast ignition by use of a strong external DC magnetic field. The second part concerns laboratory modeling of some astrophysical phenomena, including 1) studies of the topological structure of magnetic reconnection/annihilation that relates closely to geomagnetic substorms, loop-top X-ray source and mass ejection in solar flares, and 2) magnetic field generation and evolution in collisionless shock formation.
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页数：6
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