Polarization of thermal bremsstrahlung emission due to electron pressure anisotropy
Astrophysical plasmas are typically magnetized, with the Larmor radii of the charged particles many orders of magnitude smaller than their collisional mean free paths. The fundamental properties of such plasmas, e.g. conduction and viscosity, may depend on the instabilities driven by the anisotropy...
| Egile Nagusiak: | , , , |
|---|---|
| Formatua: | Journal article |
| Argitaratua: |
Oxford University Press
2016
|