The thermo magnetic instability in hot viscose plasmas
Abstract
Magnetic Rotational Instability (MRI) can not performed well in accretion disks with strong magnetic field. Studies have indicated a new type of instability called thermomagnetic instability (TMI) in systems where Nernst coefficient and gradient temperature were considered. Nernst coefficient would appear if Boltzman equation could be expanded through
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- October 2017
- DOI:
- 10.1007/s10509-017-3174-0
- Bibcode:
- 2017Ap&SS.362..197H
- Keywords:
-
- Viscosity;
- Self gravity;
- Accretion disks