Laboratory astrophysics with laser-driven strong magnetic fields in China
In this paper, the recent studies of laboratory astrophysics with strong magnetic fields in China have been reviewed. On the Shenguang-II laser facility of the National Laboratory on High-Power Lasers and Physics, a laser-driven strong magnetic field up to 200 T has been achieved. The experiment was...
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Veröffentlicht in: | High power laser science and engineering 2016, Vol.4 (3), p.67-70, Article e27 |
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creator | Wang, Fei-Lu Pei, Xiao-Xing Han, Bo Wei, Hui-Gang Yuan, Da-Wei Liang, Gui-Yun Zhao, Gang Zhong, Jia-Yong Zhang, Zhe Zhu, Bao-Jun Li, Yan-Fei Li, Fang Li, Yu-Tong Zeng, Si-Liang Zou, Shi-Yang Zhang, Jie |
description | In this paper, the recent studies of laboratory astrophysics with strong magnetic fields in China have been reviewed. On the Shenguang-II laser facility of the National Laboratory on High-Power Lasers and Physics, a laser-driven strong magnetic field up to 200 T has been achieved. The experiment was performed to model the interaction of solar wind with dayside magnetosphere. Also the low beta plasma magnetic reconnection (MR) has been studied. Theoretically, the model has been developed to deal with the atomic structures and processes in strong magnetic field. Also the study of shock wave generation in the magnetized counter-streaming plasmas is introduced. |
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Also the study of shock wave generation in the magnetized counter-streaming plasmas is introduced.</description><subject>Accretion disks</subject><subject>Aluminum</subject><subject>Astrophysics</subject><subject>Atomic structure</subject><subject>Computational mathematics</subject><subject>Experiments</subject><subject>HPLSE 2016</subject><subject>Laboratories</subject><subject>Lasers</subject><subject>Magnetic fields</subject><subject>Magnetospheres</subject><subject>Plasmas</subject><subject>Solar generators</subject><subject>Solar wind</subject><subject>Star & galaxy formation</subject><subject>Wave generation</subject><issn>2095-4719</issn><issn>2052-3289</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>IKXGN</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNptkE1LAzEQhoMoWGpP_oGAR9mazyY5SvGjUPCi55Bks7uR7e422Sr992ZpEQ-eZoZ5ZuadF4BbjJYYYfHQDO2SILxaEnEBZgRxUlAi1eWUK14wgdU1WKQULCKMcq4InYHN1tg-mrGPR2jSGPuhOabgEvwOYwNbk3wsyhi-fAenblfDnak7PwYHq-DbMsHQwXUTOnMDrirTJr84xzn4eH56X78W27eXzfpxWzgq0VhUlq8Q9gwrQaQVpLSEOM-t5xVhnlVKViVywqoKC5TLUlLjlMOSc2MtFXQO7k57h9jvDz6N-rM_xC6f1FgqRTnFYqLuT5SLfUrRV3qIYWfiUWOkJ7t0tktPdmky0fRMN_nFfejqXzyrRGIlKUdMMsUZkxznLMvJU8V5yuxsDGXt_0j558oPCnd75w</recordid><startdate>2016</startdate><enddate>2016</enddate><creator>Wang, Fei-Lu</creator><creator>Pei, Xiao-Xing</creator><creator>Han, Bo</creator><creator>Wei, Hui-Gang</creator><creator>Yuan, Da-Wei</creator><creator>Liang, Gui-Yun</creator><creator>Zhao, Gang</creator><creator>Zhong, Jia-Yong</creator><creator>Zhang, Zhe</creator><creator>Zhu, Bao-Jun</creator><creator>Li, Yan-Fei</creator><creator>Li, Fang</creator><creator>Li, Yu-Tong</creator><creator>Zeng, Si-Liang</creator><creator>Zou, Shi-Yang</creator><creator>Zhang, Jie</creator><general>Cambridge University Press</general><scope>IKXGN</scope><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>~WA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>2016</creationdate><title>Laboratory astrophysics with laser-driven strong magnetic fields in China</title><author>Wang, Fei-Lu ; 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On the Shenguang-II laser facility of the National Laboratory on High-Power Lasers and Physics, a laser-driven strong magnetic field up to 200 T has been achieved. The experiment was performed to model the interaction of solar wind with dayside magnetosphere. Also the low beta plasma magnetic reconnection (MR) has been studied. Theoretically, the model has been developed to deal with the atomic structures and processes in strong magnetic field. Also the study of shock wave generation in the magnetized counter-streaming plasmas is introduced.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/hpl.2016.27</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Accretion disks Aluminum Astrophysics Atomic structure Computational mathematics Experiments HPLSE 2016 Laboratories Lasers Magnetic fields Magnetospheres Plasmas Solar generators Solar wind Star & galaxy formation Wave generation |
title | Laboratory astrophysics with laser-driven strong magnetic fields in China |
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