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...
Үндсэн зохиолчид: | Komarov, S, Khabibullin, I, Churazov, E, Schekochihin, A |
---|---|
Формат: | Journal article |
Хэвлэсэн: |
Oxford University Press
2016
|
Ижил төстэй зүйлс
Ижил төстэй зүйлс
-
Polarization of Sunyaev-Zeldovich signal due to electron pressure anisotropy in galaxy clusters
-н: Khabibullin, I, зэрэг
Хэвлэсэн: (2017) -
Thermal conduction in a mirror-unstable plasma
-н: Komarov, S, зэрэг
Хэвлэсэн: (2016) -
Self-inhibiting thermal conduction in a high-β,
whistler-unstable plasma
-н: Komarov, S, зэрэг
Хэвлэсэн: (2018) -
Effect of bremsstrahlung radiation emission on fast electrons in plasmas
-н: O Embréus, зэрэг
Хэвлэсэн: (2016-01-01) -
The energy and angle distribution of Bremsstrahlung due to monoenergetic electrons
-н: O'Dell, Austin Almond, 1933-
Хэвлэсэн: (2012)