Abstract
For an understanding of many aeronomic processes, diffusion coefficients D. heat conductivities κ. and viscosities η are needed. To study the propagation of electromagnetic waves through a planetary atmosphere, the electrical conductivity σ of the atmosphere must be known. Since the motion of charged particles is strongly influenced by a magnetic field B pervading the plasma, e.g., the Earth’s magnetic field B ♀ the atmospheric plasma is an anisotropic medium with B := B/B as distinguished direction. Therefore the transport coefficients D. K. and σ for charged particles are tensors of second rank, the viscosity is a fourth-rank tensor.
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Suchy, K. (1984). Transport Coefficients and Collision Frequencies for Aeronomic Plasmas. In: Rawer, K. (eds) Geophysik III / Geophysics III. Handbuch der Physik / Encyclopedia of Physics, vol 10 / 49 / 7. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-68531-6_2
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DOI: https://doi.org/10.1007/978-3-642-68531-6_2
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