Particle Acceleration by Turbulent Magnetohydrodynamic Reconnection

dc.contributor.authorMatthaeus, W. H.
dc.contributor.authorAmbrosiano, J. J.
dc.contributor.authorGoldstein, Melvyn
dc.date.accessioned2023-11-03T14:51:52Z
dc.date.available2023-11-03T14:51:52Z
dc.date.issued1984-10-08
dc.description.abstractTest-particle acceleration is studied in a two-dimensional, turbulent magnetohydrodynamic simulation whose initial magnetic field configuration is a periodic sheet pinch. Some test particles become trapped near large electric field in the reconnnection region for approximately an Alfvén transit time. The maximum speed attained is consistent with an analytic estimate which depends on the reconnection electric field, the Alfvén speed, and the ratio of Larmor period to the Alfvén transit time.en_US
dc.description.sponsorshipWe thank S. L. Lamkin for assisting in the preparation of the MHD field data. Helpful discussions with F. C. Jones, K. Papadopoulos, and B. U. O. Sonnerup are gratefully acknowledged. This work was supported in part by a NASA Solar Terrestrial Theory Program grant to the Goddard Space Flight Center, and NASA Grant No. NSG 7416 to The College of William and Mary. We acknowledge the support of the Laboratory for Extraterrestrial Physics, Goddard Space Flight Center, during the course of this research.
dc.description.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.53.1449en_US
dc.format.extent4 pages
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2wpep-lnua
dc.identifier.citationMatthaeus, W. H., J. J. Ambrosiano, and M. L. Goldstein. “Particle Acceleration by Turbulent Magnetohydrodynamic Reconnection.” Physical Review Letters 53, no. 15 (October 8, 1984): 1449–52. https://doi.org/10.1103/PhysRevLett.53.1449.en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.53.1449
dc.identifier.urihttp://hdl.handle.net/11603/30524
dc.language.isoen_USen_US
dc.publisherAPSen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
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.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleParticle Acceleration by Turbulent Magnetohydrodynamic Reconnectionen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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