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- W34128183 abstract "Equations for the viscosity tensor and thermal flux of a system of charged parrticles in the presence of a magnetic field were derived from Boltzmann equations. It was assumed that deviations from the local Maxwellian distribution (with macrovelocity parallel to the magnetic field) were sufficiently small, and that the distribution functions could be described fully by the usual thirteen moments. Particular examples of the solution of equations describing the behavior of viscosity tensor and thermal flux are considered. If initial conditions are such that there are no macromotions of the gas, density and pressure are constant, and the viscosity tensor and thermal flux are only time-dependent, then the solution of the relevant equations shows that the viscosity tensor components oscillate with a frequency being a multiple of the Larmor frequency and are damped simultaneously. The possibility of a steady thermal flux in the presence of a magnetic field was also investigated. Moreover, the case of two types of charged particles is considered, neglecting the disturbance of ion distribution. (Referativnyy zhurnal, Fizika, No. 10, 1962)" @default.
- W34128183 created "2016-06-24" @default.
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- W34128183 date "1961-01-01" @default.
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- W34128183 title "A CONTRIBUTION TO THE KINETIC THEORY OF RAREFIED GASES IN A MAGNETIC FIELD" @default.
- W34128183 hasPublicationYear "1961" @default.
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