Characteristics of Minor Ions and Electrons in Flux Transfer Events Observed by the Magnetospheric Multiscale Mission.

flux transfer events magnetic reconnection magnetopause

Journal

Journal of geophysical research. Space physics
ISSN: 2169-9380
Titre abrégé: J Geophys Res Space Phys
Pays: United States
ID NLM: 101661799

Informations de publication

Date de publication:
Jul 2020
Historique:
received: 07 01 2020
revised: 18 03 2020
accepted: 15 04 2020
entrez: 1 10 2020
pubmed: 2 10 2020
medline: 2 10 2020
Statut: ppublish

Résumé

In this study, the ion composition of flux transfer events (FTEs) observed within the magnetosheath proper is examined. These FTEs were observed just upstream of the Earth's postnoon magnetopause by the National Aeronautics and Space Administration (NASA) Magnetospheric Multiscale (MMS) spacecraft constellation. The minor ion characteristics are described using energy spectrograms, flux distributions, and ion moments as the constellation encountered each FTE. In conjunction with electron data and magnetic field observations, such observations provide important contextual information on the formation, topologies, and evolution of FTEs. In particular, minor ions, when combined with the field-aligned streaming of electrons, are reliable indicators of FTE topology. The observations are also placed (i) in context of the solar wind magnetic field configuration, (ii) the connection of the sampled flux tube to the ionosphere, and (iii) the location relative to the modeled reconnection line at the magnetopause. While protons and alpha particles were often depleted within the FTEs relative to the surrounding magnetosheath plasma, the He

Identifiants

pubmed: 32999806
doi: 10.1029/2020JA027778
pii: JGRA55795
pmc: PMC7507212
doi:

Types de publication

Journal Article

Langues

eng

Pagination

e2020JA027778

Informations de copyright

©2020. The Authors.

Références

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pubmed: 32999806
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Auteurs

S M Petrinec (SM)

Lockheed Martin Advanced Technology Center Palo Alto CA USA.

J L Burch (JL)

Southwest Research Institute San Antonio TX USA.

M Chandler (M)

NASA Marshall Space Flight Center Huntsville AL USA.

C J Farrugia (CJ)

Space Science Center University of New Hampshire Durham NH USA.

S A Fuselier (SA)

Southwest Research Institute San Antonio TX USA.
Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA.

B L Giles (BL)

NASA Goddard Space Flight Center Greenbelt MD USA.

R G Gomez (RG)

Southwest Research Institute San Antonio TX USA.
Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA.

J Mukherjee (J)

Southwest Research Institute San Antonio TX USA.

W R Paterson (WR)

NASA Goddard Space Flight Center Greenbelt MD USA.

C T Russell (CT)

Earth and Space Sciences University of California Los Angeles CA USA.

D G Sibeck (DG)

NASA Goddard Space Flight Center Greenbelt MD USA.

R J Strangeway (RJ)

Earth and Space Sciences University of California Los Angeles CA USA.

R B Torbert (RB)

Space Science Center University of New Hampshire Durham NH USA.

K J Trattner (KJ)

Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA.

S K Vines (SK)

The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.

C Zhao (C)

Earth and Space Sciences University of California Los Angeles CA USA.

Classifications MeSH