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MMS Observation of Magnetic Reconnection in the Turbulent Magnetosheath
Karl Franzens Univ Graz, Inst Phys, Graz, Austria.;Austrian Acad Sci, Space Res Inst, Graz, Austria.;Hungarian Acad Sci, RCAES, Geodet & Geophys Inst, Sopron, Hungary..
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Swedish Institute of Space Physics, Uppsala Division.
Austrian Acad Sci, Space Res Inst, Graz, Austria.;UCL, Mullard Space Sci Lab, Dorking, Surrey, England..
Austrian Acad Sci, Space Res Inst, Graz, Austria..
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2017 (English)In: Journal of Geophysical Research - Space Physics, ISSN 2169-9380, E-ISSN 2169-9402, Vol. 122, no 11, p. 11442-11467Article in journal (Refereed) Published
Abstract [en]

In this paper we use the full armament of the MMS (Magnetospheric Multiscale) spacecraft to study magnetic reconnection in the turbulent magnetosheath downstream of a quasi-parallel bow shock. Contrarily to the magnetopause and magnetotail cases, only a few observations of reconnection in the magnetosheath have been reported. The case study in this paper presents, for the first time, both fluid-scale and kinetic-scale signatures of an ongoing reconnection in the turbulent magnetosheath. The spacecraft are crossing the reconnection inflow and outflow regions and the ion diffusion region (IDR). Inside the reconnection outflows D shape ion distributions are observed. Inside the IDR mixing of ion populations, crescent-like velocity distributions and ion accelerations are observed. One of the spacecraft skims the outer region of the electron diffusion region, where parallel electric fields, energy dissipation/conversion, electron pressure tensor agyrotropy, electron temperature anisotropy, and electron accelerations are observed. Some of the difficulties of the observations of magnetic reconnection in turbulent plasma are also outlined.

Place, publisher, year, edition, pages
American Geophysical Union (AGU), 2017. Vol. 122, no 11, p. 11442-11467
National Category
Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:uu:diva-342091DOI: 10.1002/2017JA024535ISI: 000419938600034OAI: oai:DiVA.org:uu-342091DiVA, id: diva2:1186936
Available from: 2018-03-01 Created: 2018-03-01 Last updated: 2018-03-02Bibliographically approved

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Yordanova, EmiliyaKhotyaintsev, Yuri V.Li, WenyaGraham, Daniel B.Norgren, CeciliaVaivads, AndrisEriksson, Elin
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Swedish Institute of Space Physics, Uppsala DivisionDepartment of Physics and Astronomy
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