Coalescence of Macroscopic Flux Ropes at the Subsolar Magnetopause: Magnetospheric Multiscale Observations

dc.contributor.authorZhou, M.
dc.contributor.authorBerchem, J.
dc.contributor.authorWalker, R. J.
dc.contributor.authorEl-Alaoui, M.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authoret al
dc.date.accessioned2024-01-18T02:22:45Z
dc.date.available2024-01-18T02:22:45Z
dc.date.issued2017-08-02
dc.descriptionAuthors: - M. Zhou, J. Berchem, R. J. Walker, M. El-Alaoui, X. Deng, E. Cazzola, G. Lapenta, Melvyn Goldstein, W. R. Paterson, Y. Pang, R. E. Ergun, B. Lavraud, H. Liang, C. T. Russell, R. J. Strangeway, C. Zhao, B. L. Giles, C. J. Pollock, P.-A. Lindqvist, G. Marklund, F. D. Wilder, Y. V. Khotyaintsev, R. B. Torbert, and J. L. Burch
dc.description.abstractWe report unambiguous in situ observation of the coalescence of macroscopic flux ropes by the magnetospheric multiscale (MMS) mission. Two coalescing flux ropes with sizes of ∼ 1 RE were identified at the subsolar magnetopause by the occurrence of an asymmetric quadrupolar signature in the normal component of the magnetic field measured by the MMS spacecraft. An electron diffusion region (EDR) with a width of four local electron inertial lengths was embedded within the merging current sheet. The EDR was characterized by an intense parallel electric field, significant energy dissipation, and suprathermal electrons. Although the electrons were organized by a large guide field, the small observed electron pressure nongyrotropy may be sufficient to support a significant fraction of the parallel electric field within the EDR. Since the flux ropes are observed in the exhaust region, we suggest that secondary EDRs are formed further downstream of the primary reconnection line between the magnetosheath and magnetospheric fields.
dc.description.sponsorshipWe thank T. Phan and N. Bessho for valuable suggestions. This research was supported by NASA Magnetospheric Multiscale Mission Interdisciplinary Scientist Grant No. NNX08AO48G, NASA Grant No. NNX15AI92G, and NSF Grant No. AGS-1450864. Work in China was supported by the National Natural Science Foundation of China (NSFC) under Grants No. 41331070 and No. 41522405 and Science Foundation of Jiangxi Province (Grant No. 20142BCB23006). EC acknowledges financial support from the Leverhulme Trust Research Project Grant No. 2014-112. We thank the entire MMS team and instrument PIs for data access and support,
dc.description.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.119.055101
dc.format.extent6 pages
dc.genrejournal articles
dc.identifier.citationZhou, M., J. Berchem, R. J. Walker, M. El-Alaoui, X. Deng, E. Cazzola, G. Lapenta, et al. “Coalescence of Macroscopic Flux Ropes at the Subsolar Magnetopause: Magnetospheric Multiscale Observations.” Physical Review Letters 119, no. 5 (August 2, 2017): 055101. https://doi.org/10.1103/PhysRevLett.119.055101.
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.119.055101
dc.identifier.urihttp://hdl.handle.net/11603/31339
dc.language.isoen_US
dc.publisherAPS
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.titleCoalescence of Macroscopic Flux Ropes at the Subsolar Magnetopause: Magnetospheric Multiscale Observations
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-5317-988X

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