Reconstruction of Electron and Ion Distribution Functions in a Magnetotail Reconnection Diffusion Region

dc.contributor.authorNg, Jonathan
dc.contributor.authorChen, Li-Jen
dc.contributor.authorHakim, Ammar
dc.contributor.authorBhattacharjee, Amitava
dc.date.accessioned2021-07-28T15:29:20Z
dc.date.available2021-07-28T15:29:20Z
dc.date.issued2020-05-23
dc.description.abstractIn the diffusion region of magnetotail reconnection, particle distributions are highly structured, exhibiting triangular shapes and multiple striations that deviate dramatically from the Maxwellian distribution. Fully kinetic simulations have been demonstrated to be capable of producing the essential structures of the observed distribution functions, yet are computationally not feasible for 3D global simulations. The fluid models used for large-scale simulations, on the other hand, do not have the kinetic physics necessary for describing reconnection accurately. Our study aims to bridge fully kinetic and fluid simulations by quantifying the information required to capture the non-Maxwellian features in the distributions underlying the closures used in the fluid code. We compare the results of fully kinetic simulations with observed electron velocity distributions in a magnetotail reconnection diffusion region and use the maximum entropy model to reconstruct electron and ion distributions using various numbers of moments obtained from the simulation. Our results indicate that using only local moments, the maximum entropy model can reproduce many of the features of the distributions: (1) the electron outflow distribution with a tilted triangular structure is reproduced with 21 or more moments in agreement with Ng et al. (2018, https://doi.org/10.1063/1.5041758) and (2) counterstreaming distributions can be captured with the 35-moment model when the separation in velocity space between the populations is large.en_US
dc.description.sponsorshipThis work was supported by DOE Contract DE-AC02-09CH11466 and NSF grant AGS-1338944, DOE grant DESC0016278, NSF grant AGS-1619584, NASA grant 80NSSC18K1369. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a US Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.en_US
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/10.1029/2020JA027879en_US
dc.format.extent12 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2qze1-naxp
dc.identifier.citationNg, Jonathan et al.; Reconstruction of Electron and Ion Distribution Functions in a Magnetotail Reconnection Diffusion Region; Journal of Geophysical Research : Space Physics, 125, 7, 23 May, 2020; https://doi.org/10.1029/2020JA027879en_US
dc.identifier.urihttps://doi.org/10.1029/2020JA027879
dc.identifier.urihttp://hdl.handle.net/11603/22196
dc.language.isoen_USen_US
dc.publisherAmerican Geophysical Unionen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleReconstruction of Electron and Ion Distribution Functions in a Magnetotail Reconnection Diffusion Regionen_US
dc.typeTexten_US

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