Published February 1, 2016
| Version v1
Journal article
Magnetic field amplification by collisionless shocks in partially ionized plasmas
Creators
- 1. Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara 252-5258 (Japan)
Description
In this paper, we study the shock structures of collisionless shocks in partially ionized plasmas by means of two-dimensional hybrid simulations, where the shock is a perpendicular shock with shock velocity and the upstream ionization fraction is 0.5. We find that large density fluctuations and large magnetic field fluctuations are generated both in the upstream and downstream regions. In addition, we find that the velocity distribution of downstream hydrogen atoms has three components. The observed shock structures suggest that diffusive shock acceleration can operate at perpendicular shocks propagating into partially ionized plasmas in real three-dimensional systems.
Availability note (English)
Available from http://dx.doi.org/10.3847/0004-637X/817/2/137Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 817
- Journal Issue
- 2
- Series
- Since 2009, the country of publication for this journal is the UK.
- Journal Page Range
- [5 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51049404
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCELERATION; ATOMS; COMPUTERIZED SIMULATION; COSMIC RADIATION; DENSITY; DISTRIBUTION; FLUCTUATIONS; HYDROGEN; IONIZATION; MAGNETIC FIELDS; PLASMA; SHOCK WAVES; SUPERNOVA REMNANTS; THREE-DIMENSIONAL CALCULATIONS; TURBULENCE; VELOCITY
- Descriptors DEC
- COSMIC RADIO SOURCES; ELEMENTS; IONIZING RADIATIONS; NONMETALS; PHYSICAL PROPERTIES; RADIATIONS; SIMULATION; VARIATIONS