Structure of a Perturbed Magnetic Reconnection Electron Diffusion Region in the Earth's Magnetotail.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
19 Nov 2021
Historique:
received: 28 03 2021
revised: 22 09 2021
accepted: 07 10 2021
entrez: 3 12 2021
pubmed: 4 12 2021
medline: 4 12 2021
Statut: ppublish

Résumé

We report in situ observations of an electron diffusion region (EDR) and adjacent separatrix region in the Earth's magnetotail. We observe significant magnetic field oscillations near the lower hybrid frequency which propagate perpendicularly to the reconnection plane. We also find that the strong electron-scale gradients close to the EDR exhibit significant oscillations at a similar frequency. Such oscillations are not expected for a crossing of a steady 2D EDR, and can be explained by a complex motion of the reconnection plane induced by current sheet kinking propagating in the out-of-reconnection-plane direction. Thus, all three spatial dimensions have to be taken into account to explain the observed perturbed EDR crossing. These results shed light on the interplay between magnetic reconnection and current sheet drift instabilities in electron-scale current sheets and highlight the need for adopting a 3D description of the EDR, going beyond the two-dimensional and steady-state conception of reconnection.

Identifiants

pubmed: 34860109
doi: 10.1103/PhysRevLett.127.215101
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

215101

Auteurs

G Cozzani (G)

Swedish Institute of Space Physics, Uppsala 75121, Sweden.

Yu V Khotyaintsev (YV)

Swedish Institute of Space Physics, Uppsala 75121, Sweden.

D B Graham (DB)

Swedish Institute of Space Physics, Uppsala 75121, Sweden.

J Egedal (J)

Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.

M André (M)

Swedish Institute of Space Physics, Uppsala 75121, Sweden.

A Vaivads (A)

Space and Plasma Physics, School of Electrical Engineering and Computer Science, KTH Royal Institute of Technology, Stockholm 11428, Sweden.

A Alexandrova (A)

Laboratoire de Physique des Plasmas, CNRS, Sorbonne Université, Université Paris-Saclay, Observatoire de Paris, École Polytechnique Institut Polytechnique de Paris, Palaiseau 91128, France.

O Le Contel (O)

Laboratoire de Physique des Plasmas, CNRS, Sorbonne Université, Université Paris-Saclay, Observatoire de Paris, École Polytechnique Institut Polytechnique de Paris, Palaiseau 91128, France.

R Nakamura (R)

Space Research Institute, Austrian Academy of Sciences, Graz 8042, Austria.

S A Fuselier (SA)

Southwest Research Institute, San Antonio, Texas 78238, USA.
University of Texas at San Antonio, San Antonio, Texas 78249, USA.

C T Russell (CT)

University of California, Los Angeles, California 90095, USA.

J L Burch (JL)

Southwest Research Institute, San Antonio, Texas 78238, USA.

Classifications MeSH