Magnetic Field Annihilation in a Magnetotail Electron Diffusion Region With Electron-Scale Magnetic Island.

electron diffusion region magnetic diffusion magnetic field annihilation magnetic island magnetic reconnection magnetotail

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 2022
Historique:
received: 22 02 2022
revised: 27 05 2022
accepted: 20 06 2022
entrez: 17 10 2022
pubmed: 18 10 2022
medline: 18 10 2022
Statut: ppublish

Résumé

We present observations in Earth's magnetotail by the Magnetospheric Multiscale spacecraft that are consistent with magnetic field annihilation, rather than magnetic topology change, causing fast magnetic-to-electron energy conversion in an electron-scale current sheet. Multi-spacecraft analysis for the magnetic field reconstruction shows that an electron-scale magnetic island was embedded in the observed electron diffusion region (EDR), suggesting an elongated shape of the EDR. Evidence for the annihilation was revealed in the form of the island growing at a rate much lower than expected for the standard X-type geometry of the EDR, which indicates that magnetic flux injected into the EDR was not ejected from the X-point or accumulated in the island, but was dissipated in the EDR. This energy conversion process is in contrast to that in the standard EDR of a reconnecting current sheet where the energy of antiparallel magnetic fields is mostly converted to electron bulk-flow energy. Fully kinetic simulation also demonstrates that an elongated EDR is subject to the formation of electron-scale magnetic islands in which fast but transient annihilation can occur. Consistent with the observations and simulation, theoretical analysis shows that fast magnetic diffusion can occur in an elongated EDR in the presence of nongyrotropic electron effects. We suggest that the annihilation in elongated EDRs may contribute to the dissipation of magnetic energy in a turbulent collisionless plasma.

Identifiants

pubmed: 36248013
doi: 10.1029/2022JA030408
pii: JGRA57268
pmc: PMC9541864
doi:

Types de publication

Journal Article

Langues

eng

Pagination

e2022JA030408

Informations de copyright

© 2022. The Authors.

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Auteurs

H Hasegawa (H)

Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Sagamihara Japan.

R E Denton (RE)

Department of Physics and Astronomy Dartmouth College Hanover NH USA.

T K M Nakamura (TKM)

Space Research Institute Austrian Academy of Sciences Graz Austria.
Institute of Physics University of Graz Graz Austria.

K J Genestreti (KJ)

Southwest Research Institute Durham NH USA.

T D Phan (TD)

Space Sciences Laboratory University of California Berkeley CA USA.

R Nakamura (R)

Space Research Institute Austrian Academy of Sciences Graz Austria.

K-J Hwang (KJ)

Southwest Research Institute San Antonio TX USA.

N Ahmadi (N)

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

Q Q Shi (QQ)

Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment Institute of Space Sciences Shandong University Weihai China.

M Hesse (M)

NASA Ames Research Center Moffett Field CA USA.

J L Burch (JL)

Southwest Research Institute San Antonio TX USA.

J M Webster (JM)

Southwest Research Institute San Antonio TX USA.

R B Torbert (RB)

Institute of Physics University of Graz Graz Austria.
Physics Department University of New Hampshire Durham NH USA.

B L Giles (BL)

NASA Goddard Space Flight Center Greenbelt MD USA.

D J Gershman (DJ)

NASA Goddard Space Flight Center Greenbelt MD USA.

C T Russell (CT)

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

R J Strangeway (RJ)

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

H Y Wei (HY)

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

P-A Lindqvist (PA)

Royal Institute of Technology Stockholm Sweden.

Y V Khotyaintsev (YV)

Swedish Institute of Space Physics Uppsala Sweden.

R E Ergun (RE)

Department of Astrophysical and Planetary Sciences University of Colorado Boulder CO USA.

Y Saito (Y)

Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Sagamihara Japan.

Classifications MeSH