Magnetic reconnection driven by intense lasers

被引:9
作者
Zhong, Jiayong [1 ,2 ]
Yuan, Xiaoxia [1 ]
Han, Bo [1 ]
Sun, Wei [1 ]
Ping, Yongli [1 ]
机构
[1] Beijing Normal Univ, Dept Astron, 19,Xinjiekouwai St, Beijing 100875, Peoples R China
[2] Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China
来源
HIGH POWER LASER SCIENCE AND ENGINEERING | 2018年 / 6卷
基金
中国国家自然科学基金;
关键词
high energy density physics; laser plasmas interaction; plasmas astrophysics; X-RAY SOURCE; ELECTRON ACCELERATION; RELATIVISTIC PICKUP; SOLAR-FLARE; MODEL; FIELDS; ENERGY; CONFINEMENT; GENERATION; IONIZATION;
D O I
10.1017/hpl.2018.39
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Laser-driven magnetic reconnection (LDMR) occurring with self-generated B fields has been experimentally and theoretically studied extensively, where strong B fields of more than megagauss are spontaneously generated in high-power laser-plasma interactions, which are located on the target surface and produced by non-parallel temperature and density gradients of expanding plasmas. For properties of the short-lived and strong B fields in laser plasmas, LDMR opened up a new territory in a parameter regime that has never been exploited before. Here we review the recent results of LDMR taking place in both high and low plasma beta environments. We aim to understand the basic physics processes of magnetic reconnection, such as particle accelerations, scale of the diffusion region, and guide field effects.Some applications of experimental results are also given especially for space and solar plasmas.
引用
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页数:17
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