Published September 1, 2021 | Version v1
Journal article

Kinetic Imprints of Ion Acceleration in Collisionless Magnetic Reconnection

  • 1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences (China)
  • 2. Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Pessac (France)

Description

Fast collisionless magnetic reconnection implies fast energy conversion. The main form of energy conversion in magnetic reconnection concerns bulk ion acceleration with resulting ion jets. Based on theoretical analysis and MMS data, we examine the kinetic imprints of ion in the context of fast reconnection rates. The ion kinetic imprints we analyze in MMS observations include ion beams toward the X-line and distorted velocity distributions in reconnection jets. The distorted ion velocity distributions lead to a bipolar reversal in an off-diagonal element of the pressure tensor across the X-line, supporting an enhancement of the ion-scale reconnection electric field.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4357/ac0fde

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
919
Journal Issue
1
Journal Page Range
[9 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
53076524
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S42: ENGINEERING;
Descriptors DEI
ACCELERATION; ELECTRIC FIELDS; ENERGY CONVERSION; ION BEAMS; IONS; JETS; KINETICS; MAGNETIC RECONNECTION; TENSORS; VELOCITY
Descriptors DEC
BEAMS; CHARGED PARTICLES; CONVERSION