@article{7c5060f7bef042d78f56e770126de9aa,
title = "Magnetic reconnection in partially ionized plasmas",
abstract = "Magnetic reconnection has been intensively studied in fully ionized plasmas. However, plasmas are often partially ionized in astrophysical environments. The interactions between the neutral particles and ionized plasmas might strongly affect the reconnection mechanisms. We review magnetic reconnection in partially ionized plasmas in different environments from theoretical, numerical, observational and experimental points of view.We focus on mechanisms which make magnetic reconnection fast enough to compare with observations, especially on the reconnection events in the low solar atmosphere. The heating mechanisms and the related observational evidence of the reconnection process in the partially ionized low solar atmosphere are also discussed. We describe magnetic reconnection in weakly ionized astrophysical environments, including the interstellar medium and protostellar discs. We present recent achievements about fast reconnection in laboratory experiments for partially ionized plasmas.",
keywords = "Experiment, Magnetic reconnection, Partially ionized plasmas, Simulation, Theory",
author = "Lei Ni and Hantao Ji and Murphy, {Nicholas A.} and Jonathan Jara-Almonte",
note = "Funding Information: This research is supported by NSFC grant nos. 11973083, 11573064, 11333007, 11303101 and 11403100; the Youth Innovation Promotion Association CAS 2017; the Applied Basic Research of Yunnan Province in China grant no. 2018FB009; the Yunnan Ten-Thousand Talents Plan-Young top talents; the key Laboratory of Solar Activity grant no. KLSA201812; the Strategic Priority Research Program of CAS with grant nos. XDA17040507, QYZDJ-SSWSLH012 and XDA15010900; the project of the Group for Innovation of Yunnan Province grant no. 2018HC023; the YunnanTen-Thousand Talents Plan-Yunling Scholar Project. H.J. and J.J.A. acknowledge support by the U.S. Department of Energy Office of Fusion Energy Sciences under Contract No. DE-AC02-09CH11466. N.A.M. acknowledges support from the U.S. NSF grant no. 1931388. Funding Information: Data accessibility. This article has no additional data. Authors{\textquoteright} contributions. L.N. wrote most of §§1–3 and 6. N.M. wrote most of §4. H.J. and J.J.A. wrote most of §5. All authors contributed to revisions of the manuscript. Competing interests. We declare we have no competing interests. Funding. This research is supported by NSFC grant nos. 11973083, 11573064, 11333007, 11303101 and 11403100; the Youth Innovation Promotion Association CAS 2017; the Applied Basic Research of Yunnan Province in China grant no. 2018FB009; the Yunnan Ten-Thousand Talents Plan-Young top talents; the key Laboratory of Solar Activity grant no. KLSA201812; the Strategic Priority Research Program of CAS with grant nos. XDA17040507, QYZDJ-SSWSLH012 and XDA15010900; the project of the Group for Innovation of Yunnan Province grant no. 2018HC023; the YunnanTen-Thousand Talents Plan-Yunling Scholar Project. H.J. and J.J.A. acknowledge support by the U.S. Department of Energy Office of Fusion Energy Sciences under Contract No. DE-AC02-09CH11466. N.A.M. acknowledges support from the U.S. NSF grant no. 1931388. Acknowledgements. The authors are grateful to all the referees for their valuable comments and suggestions. L.N. would like to thank Dr Jun Lin for his helpful discussions. Publisher Copyright: {\textcopyright} 2020 The Author(s) Published by the Royal Society. All rights reserved.",
year = "2020",
month = apr,
day = "1",
doi = "10.1098/rspa.2019.0867",
language = "English (US)",
volume = "476",
journal = "PROC. R. SOC. - A.",
issn = "0950-1207",
publisher = "Royal Society of London",
number = "2236",
}