Published September 1, 2021
| Version v1
Journal article
Kinetic Imprints of Ion Acceleration in Collisionless Magnetic Reconnection
Creators
- 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/ac0fdeAdditional 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