Particle-in-cell simulations of collisionless perpendicular shocks driven at a laser-plasma device

被引:1
作者
Hao, Yufei [1 ,2 ,3 ,4 ]
Yang, Zhongwei [3 ]
Tang, Huibo [2 ,4 ]
Kong, Xiangliang [5 ]
Shan, Lican [6 ]
机构
[1] Chinese Acad Sci, Key Lab Planetary Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
[2] Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China
[3] Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing 100190, Peoples R China
[4] CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R China
[5] Shandong Univ, Inst Space Sci, Inst Frontier & Interdisciplinary Sci, Sch Space Sci & Phys, Weihai 264209, Shandong, Peoples R China
[6] Chinese Acad Sci, Inst Geol & Geophys, CAS Engn Lab Deep Resources Equipment & Technol, Beijing 100029, Peoples R China
基金
国家重点研发计划;
关键词
HYBRID SIMULATIONS; WAVES; ACCELERATION; DISSIPATION; DOWNSTREAM;
D O I
10.1063/5.0142363
中图分类号
TB3 [工程材料学];
学科分类号
0805 ; 080502 ;
摘要
Experiments of generation of quasi-perpendicular collisionless shocks driven by laser plasma were performed at the Shenguang-II laser facility with intense lasers. Here, using 1D a particle-in-cell simulation code including protons, carbon ions, and electrons, we investigate the experimental shock formation via the interaction between the laser-ablated piston and ambient plasma magnetized by a large pre-existing magnetic field and the associated ion dynamics in more detail. Simulation results show that, given enough time and space, ambient protons and carbon ions can be reflected at the piston-ambient interface successively, which leads to the formation of corresponding shocks before the piston and interface. Electric fields associated with the initial interaction known as Larmor coupling and the shocks may accelerate ambient protons, carbon ions reflected at the interface or shocks, and piston ones transmitted to the ambient region before shock formation.
引用
收藏
页数:9
相关论文
共 57 条
  • [1] Angelopoulos V, 2008, SPACE SCI REV, V141, P5, DOI 10.1007/s11214-008-9336-1
  • [2] Axford W. I., 1977, P 15 INT COSM RAY C, P132
  • [3] ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1.
    BELL, AR
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 182 (01) : 147 - 156
  • [4] PARTICLE ACCELERATION BY ASTROPHYSICAL SHOCKS
    BLANDFORD, RD
    OSTRIKER, JP
    [J]. ASTROPHYSICAL JOURNAL, 1978, 221 (01) : L29 - L32
  • [5] Bondarenko AS, 2017, NAT PHYS, V13, P573, DOI [10.1038/NPHYS4041, 10.1038/nphys4041]
  • [6] Magnetospheric Multiscale Overview and Science Objectives
    Burch, J. L.
    Moore, T. E.
    Torbert, R. B.
    Giles, B. L.
    [J]. SPACE SCIENCE REVIEWS, 2016, 199 (1-4) : 5 - 21
  • [7] Plasmoid Ejection and Secondary Current Sheet Generation from Magnetic Reconnection in Laser-Plasma Interaction
    Dong, Quan-Li
    Wang, Shou-Jun
    Lu, Quan-Ming
    Huang, Can
    Yuan, Da-Wei
    Liu, Xun
    Lin, Xiao-Xuan
    Li, Yu-Tong
    Wei, Hui-Gang
    Zhong, Jia-Yong
    Shi, Jian-Rong
    Jiang, Shao-En
    Ding, Yong-Kun
    Jiang, Bo-Bin
    Du, Kai
    He, Xian-Tu
    Yu, M. Y.
    Liu, C. S.
    Wang, Shui
    Tang, Yong-Jian
    Zhu, Jian-Qiang
    Zhao, Gang
    Sheng, Zheng-Ming
    Zhang, Jie
    [J]. PHYSICAL REVIEW LETTERS, 2012, 108 (21)
  • [8] The Cluster mission - Introduction
    Escoubet, CP
    Fehringer, M
    Goldstein, M
    [J]. ANNALES GEOPHYSICAE, 2001, 19 (10-12) : 1197 - 1200
  • [9] FORMATION AND STRUCTURE OF ELECTROSTATIC COLLISIONLESS SHOCKS
    FORSLUND, DW
    SHONK, CR
    [J]. PHYSICAL REVIEW LETTERS, 1970, 25 (25) : 1699 - &
  • [10] COLLISIONLESS DISSIPATION IN QUASI-PERPENDICULAR SHOCKS
    FORSLUND, DW
    QUEST, KB
    BRACKBILL, JU
    LEE, K
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1984, 89 (NA4): : 2142 - 2150