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...

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Main Authors: Komarov, S, Khabibullin, I, Churazov, E, Schekochihin, A
格式: Journal article
出版: Oxford University Press 2016

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