@article{f88d8e2a15dc43a1b56d2cae7e3821a5,
title = "Modeling the interaction of solar wind with a dipole magnetic field with Shenguang II intense lasers",
abstract = "The interaction of solar wind with a dipole magnetic field is modeled in a laboratory setting with a small cylindrical permanent magnet and magnetized plasma driven by intense lasers. The result shows a potential application in the understanding of Earth's magnetosphere near the pole region. Some significant features are observed in our experiments, such as magnetic reconnection and repulsion, which agree well with magnetohydrodynamics (MHD) simulation results.",
author = "K. Zhang and Zhong, {J. Y.} and Wang, {J. Q.} and Pei, {X. X.} and Wei, {H. G.} and Yuan, {D. W.} and Yang, {Z. W.} and C. Wang and F. Li and B. Han and Yin, {C. L.} and Liao, {G. Q.} and Y. Fang and S. Yang and Yuan, {X. H.} and Y. Sakawa and T. Morita and Cao, {Z. R.} and Jiang, {S. E.} and Ding, {Y. K.} and Y. Kuramitsu and Liang, {G. Y.} and Wang, {F. L.} and Li, {Y. T.} and Zhu, {J. Q.} and J. Zhang and G. Zhao",
note = "Funding Information: The authors are very much grateful to the SG2 operation staffs and the target preparation staffs for valuable help and support. This work is supported by the National Basic Research Program of China (973 program) (Grant Nos. 2013CBA01500 ), and the National Natural Science Foundation of China (Grant Nos. 11135012, 11220101002, 11273033 , 11205015 ) and Beijing Nova Program ( Z131109000413050 ). Publisher Copyright: {\textcopyright} 2014 Elsevier B.V.",
year = "2015",
month = dec,
day = "1",
doi = "10.1016/j.hedp.2014.11.001",
language = "English",
volume = "17",
pages = "32--37",
journal = "High Energy Density Physics",
issn = "1574-1818",
publisher = "Elsevier",
}