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作 者:Jiayong Zhong Xiaoxia Yuan Bo Han Wei Sun Yongli Ping
机构地区:[1]Department of Astronomy, Beijing Normal University [2]IFSA Collaborative Innovation Center, Shanghai Jiao Tong University
出 处:《High Power Laser Science and Engineering》2018年第3期85-101,共17页高功率激光科学与工程(英文版)
基 金:supported by the Science Challenge Project(No.TZ2016005);the National Basic Research Program of China(No.2013CBA01503);the National Natural Science Foundation of China(Nos.10905004,11220101002,and11622323);the Fundamental Research Funds for the Central Universities
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 highpower 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.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.
关 键 词:high energy density physics laser plasmas interaction plasmas astrophysics
分 类 号:TN24[电子电信—物理电子学]
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