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) |
|---|---|
| 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
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