NONRELATIVISTIC COLLISIONLESS SHOCKS IN WEAKLY MAGNETIZED ELECTRON-ION PLASMAS: TWO-DIMENSIONAL PARTICLE-IN-CELL SIMULATION OF PERPENDICULAR SHOCK
Journal Article
·
· Astrophysical Journal
- Institute of Laser Engineering, Osaka University, 2-6 Yamada-oka, Suita, Osaka 565-0871 (Japan)
A two-dimensional particle-in-cell simulation is performed to investigate weakly magnetized perpendicular shocks with a magnetization parameter of {sigma} = 6 x 10{sup -5}, which is equivalent to a high Alfven Mach number M{sub A} of {approx}130. It is shown that current filaments form in the foot region of the shock due to the ion-beam-Weibel instability (or the ion filamentation instability) and that they generate a strong magnetic field there. In the downstream region, these current filaments also generate a tangled magnetic field that is typically 15 times stronger than the upstream magnetic field. The thermal energies of electrons and ions in the downstream region are not in equipartition and their temperature ratio is T{sub e}/T{sub i} {approx} 0.3-0.4. Efficient electron acceleration was not observed in our simulation, although a fraction of the ions are accelerated slightly on reflection at the shock. The simulation results agree very well with the Rankine-Hugoniot relations. It is also shown that electrons and ions are heated in the foot region by the Buneman instability (for electrons) and the ion-acoustic instability (for both electrons and ions). However, the growth rate of the Buneman instability is significantly reduced due to the relatively high temperature of the reflected ions. For the same reason, ion-ion streaming instability does not grow in the foot region.
- OSTI ID:
- 21464821
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 721; ISSN ASJOAB; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
Nonrelativistic perpendicular shocks modeling young supernova remnants: Nonstationary dynamics and particle acceleration at forward and reverse shocks
Electron Pre-acceleration at Nonrelativistic High-Mach-number Perpendicular Shocks
PARTICLE ACCELERATION IN RELATIVISTIC MAGNETIZED COLLISIONLESS ELECTRON-ION SHOCKS
Journal Article
·
Sun Mar 20 00:00:00 EDT 2016
· Astrophysical Journal
·
OSTI ID:22890124
Electron Pre-acceleration at Nonrelativistic High-Mach-number Perpendicular Shocks
Journal Article
·
Wed Sep 20 00:00:00 EDT 2017
· Astrophysical Journal
·
OSTI ID:22875766
PARTICLE ACCELERATION IN RELATIVISTIC MAGNETIZED COLLISIONLESS ELECTRON-ION SHOCKS
Journal Article
·
Sun Jan 09 23:00:00 EST 2011
· Astrophysical Journal
·
OSTI ID:21567676
Related Subjects
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
79 ASTRONOMY AND ASTROPHYSICS
ASTROPHYSICS
BEAMS
COSMIC RADIO SOURCES
DIMENSIONLESS NUMBERS
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
ION BEAMS
LEPTONS
MACH NUMBER
MAGNETIC FIELDS
MAGNETIZATION
PHYSICS
SHOCK WAVES
SIMULATION
SUPERNOVA REMNANTS
TWO-DIMENSIONAL CALCULATIONS
VELOCITY
GENERAL PHYSICS
79 ASTRONOMY AND ASTROPHYSICS
ASTROPHYSICS
BEAMS
COSMIC RADIO SOURCES
DIMENSIONLESS NUMBERS
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
ION BEAMS
LEPTONS
MACH NUMBER
MAGNETIC FIELDS
MAGNETIZATION
PHYSICS
SHOCK WAVES
SIMULATION
SUPERNOVA REMNANTS
TWO-DIMENSIONAL CALCULATIONS
VELOCITY