Abstract
Reconnection of magnetic field lines for a wide range of parameters in the relativistic regime is considered. A newly developed covariant fluid model for magnetized plasmas, incorporating pressure anisotropy, is used to expand the study of the Petschek-type reconnection in a pair-plasma governed by slow-mode shocks. The plasma parameters are found to be strongly modified by anisotropy on both sides of the shock.
Original language | English (US) |
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Pages (from-to) | 335-341 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 403 |
Issue number | 1 |
DOIs | |
State | Published - Mar 2010 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Magnetic fields
- MHD
- Shock waves