Bow shocks formed by a high-speed laser-driven plasma cloud interacting with a cylinder obstacle
A bow shock is formed in the interaction of a high-speed laser-driven plasma cloud with a cylinder obstacle. Its temporal and spatial structures are observed by shadowgraphy and interferometry. The width of the shock transition region is - 50 μm, comparable to the ion–ion collision mean free path, w...
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| Published in | Chinese physics B Vol. 26; no. 5; pp. 279 - 283 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
01.05.2017
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| Subjects | |
| Online Access | Get full text |
| ISSN | 1674-1056 2058-3834 |
| DOI | 10.1088/1674-1056/26/5/055202 |
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| Abstract | A bow shock is formed in the interaction of a high-speed laser-driven plasma cloud with a cylinder obstacle. Its temporal and spatial structures are observed by shadowgraphy and interferometry. The width of the shock transition region is - 50 μm, comparable to the ion–ion collision mean free path, which indicates that collision is dominated in the shock probably. The Mach-number of the ablating plasma cloud is ～ 15 at first, and decreases with time resulting in a changing shock structure. A two-dimension hydrodynamics code, USim, is used to simulate the interaction process. The simulated shocks can well reproduce the observed. |
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| AbstractList | A bow shock is formed in the interaction of a high-speed laser-driven plasma cloud with a cylinder obstacle. Its temporal and spatial structures are observed by shadowgraphy and interferometry. The width of the shock transition region is - 50 μm, comparable to the ion–ion collision mean free path, which indicates that collision is dominated in the shock probably. The Mach-number of the ablating plasma cloud is ～ 15 at first, and decreases with time resulting in a changing shock structure. A two-dimension hydrodynamics code, USim, is used to simulate the interaction process. The simulated shocks can well reproduce the observed. |
| Author | 李彦霏 李玉同 袁大伟 李芳 朱保君 张喆 仲佳勇 韩波 魏会冈 裴晓星 赵家瑞 刘畅 原晓霞 廖国前 Yong-Joo Rhee 鲁欣 华能 朱宝强 朱健强 方智恒 黄秀光 傅思祖 赵刚 张杰 |
| AuthorAffiliation | Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China Department of Astronomy, Beijing Normal University, Beijing 100875, China Center for Relativistic Laser Science, Institute for Basic Science, Gwangju 61005, Korea National Laboratory on High Power Lasers and Physics, Shanghai 201800, China Shanghai Institute of Laser Plasma, Chinese Academy of Engineering Physics, Shanghai 201800, China Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China Collaborative Innovation Centre of IFSA （CICIFSA）, Shanghai Jiao Tong University, Shanghai 200240, China School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China |
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| Cites_doi | 10.1086/apjs.2000.127.issue-2 10.1038/nphys1790 10.1103/PhysRevLett.25.1699 10.1007/s11433-013-5343-7 10.1016/j.asr.2007.04.050 10.1088/0004-637X/815/1/46 pii/S2468080X16300310 10.1029/1999GL010703 10.1086/590387 10.1029/JA092iA08p08545 10.1063/1.1138755 10.1016/j.hedp.2011.11.001 10.1029/JA087iA07p05063 10.1063/1.3694124 10.1086/307293 10.1063/1.4944928 10.1103/PhysRevA.38.1363 10.1016/j.hedp.2014.11.001 10.1103/PhysRevLett.92.015002 10.1038/nature02960 S209547191600027X 10.1103/PhysRevLett.96.045005 10.1016/j.hedp.2013.01.008 10.1029/2006GL027799 10.1103/PhysRevLett.94.095005 10.1093/pasj/psu162 10.1016/j.asr.2014.03.015 10.1088/0004-637X/805/2/186 10.1038/ncomms13081 10.1086/498846 10.1038/nature06210 10.1029/JA087iA07p05081 |
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| Notes | A bow shock is formed in the interaction of a high-speed laser-driven plasma cloud with a cylinder obstacle. Its temporal and spatial structures are observed by shadowgraphy and interferometry. The width of the shock transition region is - 50 μm, comparable to the ion–ion collision mean free path, which indicates that collision is dominated in the shock probably. The Mach-number of the ablating plasma cloud is ～ 15 at first, and decreases with time resulting in a changing shock structure. A two-dimension hydrodynamics code, USim, is used to simulate the interaction process. The simulated shocks can well reproduce the observed. Yan-Fei Li1,9, Yu-Tong Li1,8,9, Da-Wei Yuan2, Fang Li1, Bao-Jun Zhu1,9, Zhe Zhang1, Jia-Yong Zhong3,8, Bo Han2,3, Hui-Gang Wei2, Xiao-Xing Pei2, Jia-Rui Zhao1, Chang Liu3, Xiao-Xia Yuan3, Guo-Qian Liao1, Yong-Joo Rhee4, Xin Lu1,9, Neng Hua5, Bao-Qiang Zhu5, Jian-Qiang Zhu5,8, Zhi-Heng Fang6, Xiu-Guang Huang6,8, Si-Zu Fu6,8, Gang Zhao2,8, Jie Zhang7,8（1Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China ; 2National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China ; 3 Department of Astronomy, Beijing Normal University, Beijing 100875, China ;4 Center for Relativistic Laser Science, Institute for Basic Science, Gwangju 61005, Korea ; 5National Laboratory on High Power Lasers and Physics, Shanghai 201800, China ; 6 Shanghai Institute of Laser Plasma, Chinese Academy of Engineering Physics, Shanghai 201800, China; 7Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China ;8 Collaborative Innovation Centre of IFSA （CICIFSA）, Shanghai Jiao Tong University, Shanghai 200240, China ; 9School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China） cylinder interacting cloud obstacle collision interferometry hydrodynamics dominated upstream supersonic 11-5639/O4 |
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| Title | Bow shocks formed by a high-speed laser-driven plasma cloud interacting with a cylinder obstacle |
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