Identifying the electron diffusion region in a realistic simulation of Earth's magnetotail

dc.contributor.authorAshour-Abdalla, Maha
dc.contributor.authorLapenta, Giovanni
dc.contributor.authorWalker, Raymond
dc.contributor.authorEl-Alaoui, Mostafa
dc.contributor.authorLiang, Haoming
dc.contributor.authorZhou, Meng
dc.contributor.authorBerchem, Jean
dc.contributor.authorGoldstein, Melvyn
dc.date.accessioned2024-01-17T11:32:05Z
dc.date.available2024-01-17T11:32:05Z
dc.date.issued2016-05-22
dc.description.abstractA historic challenge to understanding geomagnetic activity is determining where in Earth's magnetotail magnetic energy is converted into particle energy and heat by magnetic reconnection. Key to unravel this fundamental process is in determining the location and extent of the electron diffusion region (EDR) where the energy conversion is initiated. We have located the EDR during a substorm on 15 February 2008 by using a combination of global magnetohydrodynamic (MHD) and particle-in-cell (PIC) simulations. Solar wind data were used as input into the MHD simulation, which provided the initial and boundary conditions for the PIC calculation. The simulated reconnection rate was episodic with magnetic reconnection occurring every few seconds. The reconnection site moved several Earth radii in a few minutes. A parameter that measures the breakdown of electron gyrotropy about the magnetic field provided the clearest location of the EDR where changes in magnetic topology and particle acceleration are initiated.
dc.description.sponsorshipThis work was supported by a Magnetospheric Multiscale Mission Interdisciplinary Scientist grant (NASA grant NNX08AO48G) at UCLA and at the Goddard Space Flight Center, a NASA Geospace grant (NNX12AD13G), NASA Heliospheric Grand Challenge grant (NNX14AI16G), and NSF grant AGS-1450864. One of the authors (G.L.) acknowledges partial support from the Belgian Space Policy IUAP grant CHARM, from KU Leuven BOF, and GOA grants and from the EC project DEEP-ER. The computations were carried out at the NASA Advanced Supercomputing Facilities (Pleiades at NAS). The data produced by the simulation are stored in HDF5 format on the NASA-NAS data server Lou and are available upon request to the authors.
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/10.1002/2016GL069355
dc.format.extent7 pages
dc.genrejournal articles
dc.identifier.citationAshour-Abdalla, M., Lapenta, G., Walker, R., El-Alaoui, M., Liang, H., Zhou, M., Berchem, J., and Goldstein, M. L. (2016), Identifying the electron diffusion region in a realistic simulation of Earth's magnetotail, Geophys. Res. Lett., 43, 6005–6011, doi:10.1002/2016GL069355.
dc.identifier.urihttps://doi.org/10.1002/2016GL069355
dc.identifier.urihttp://hdl.handle.net/11603/31315
dc.language.isoen_US
dc.publisherAGU
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.relation.ispartofUMBC Faculty Collection
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.rightsPublic Domain Mark 1.0 en
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titleIdentifying the electron diffusion region in a realistic simulation of Earth's magnetotail
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-5317-988X

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