Electron Bernstein waves driven by electron crescents near the electron diffusion region.


Journal

Nature communications
ISSN: 2041-1723
Titre abrégé: Nat Commun
Pays: England
ID NLM: 101528555

Informations de publication

Date de publication:
09 Jan 2020
Historique:
received: 26 11 2018
accepted: 05 12 2019
entrez: 11 1 2020
pubmed: 11 1 2020
medline: 11 1 2020
Statut: epublish

Résumé

The Magnetospheric Multiscale (MMS) spacecraft encounter an electron diffusion region (EDR) of asymmetric magnetic reconnection at Earth's magnetopause. The EDR is characterized by agyrotropic electron velocity distributions on both sides of the neutral line. Various types of plasma waves are produced by the magnetic reconnection in and near the EDR. Here we report large-amplitude electron Bernstein waves (EBWs) at the electron-scale boundary of the Hall current reversal. The finite gyroradius effect of the outflow electrons generates the crescent-shaped agyrotropic electron distributions, which drive the EBWs. The EBWs propagate toward the central EDR. The amplitude of the EBWs is sufficiently large to thermalize and diffuse electrons around the EDR. The EBWs contribute to the cross-field diffusion of the electron-scale boundary of the Hall current reversal near the EDR.

Identifiants

pubmed: 31919351
doi: 10.1038/s41467-019-13920-w
pii: 10.1038/s41467-019-13920-w
pmc: PMC6952373
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

141

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Auteurs

W Y Li (WY)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, 100190, Beijing, China. wyli@spaceweather.ac.cn.
Swedish Institute of Space Physics, SE-75121, Uppsala, Sweden. wyli@spaceweather.ac.cn.
State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China. wyli@spaceweather.ac.cn.

D B Graham (DB)

Swedish Institute of Space Physics, SE-75121, Uppsala, Sweden. dgraham@irfu.se.

Yu V Khotyaintsev (YV)

Swedish Institute of Space Physics, SE-75121, Uppsala, Sweden.

A Vaivads (A)

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

M André (M)

Swedish Institute of Space Physics, SE-75121, Uppsala, Sweden.

K Min (K)

Department of Astronomy and Space Science, Chungnam National University, Daejeon, 34134, Republic of Korea.

K Liu (K)

Department of Earth and Space Sciences, Southern University of Science and Technology, 518055, Shenzhen, China.

B B Tang (BB)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, 100190, Beijing, China.

C Wang (C)

State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, 100190, Beijing, China.

K Fujimoto (K)

School of Space and Environment, Beihang University, 100191, Beijing, China.

C Norgren (C)

Department of Physics and Technology, University of Bergen, 5020, Bergen, Norway.

S Toledo-Redondo (S)

Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, UPS, CNES, 31028, Toulouse, France.
Department of Electromagnetism and Electronics, University of Murcia, 30003, Murcia, Spain.

P-A Lindqvist (PA)

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

R E Ergun (RE)

Laboratory of Atmospheric and Space Physics, University of Colorado, Boulder, CO, 80303, USA.

R B Torbert (RB)

Space Science Center, University of New Hampshire, Durham, NH, 03824, USA.

A C Rager (AC)

Catholic University of America, Washington, DC, 20064, USA.
NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA.

J C Dorelli (JC)

NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA.

D J Gershman (DJ)

NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA.
Department of Astronomy, University of Maryland, College Park, MD, 20742, USA.

B L Giles (BL)

NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA.

B Lavraud (B)

Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, UPS, CNES, 31028, Toulouse, France.

F Plaschke (F)

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

W Magnes (W)

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

O Le Contel (O)

Laboratoire de Physique des Plasmas, CNRS/Ecole Polytechnique/Sorbonne Université/Univ. Paris Sud/Observatoire de Paris, 75252, Paris, France.

C T Russell (CT)

Department of Earth and Space Sciences, University of California, Los Angeles, CA, 90095, USA.

J L Burch (JL)

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

Classifications MeSH