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- W2010847057 abstract "The paper is a review of present estimates of the kinetic and transport properties of the interplanetary medium. It is pointed out that the effective mean free paths of interplanetary ions and electrons are effectively small compared to the scale of the system either because of Coulomb collisions or because of dynamical instability of the gas. Numerical expressions are given for the mean free path for Coulomb collisions, the electrical conductivity, the thermal conductivity, the viscosity, electromagnetic emission rates, recombination and ionization times and the charge exchange cross-sections. The magnetic Reynolds number of the solar wind proves to be large, the Reynolds number is not very large and the Prandtl number is small. All stationary atoms and ions are swept out of the solar system by the solar wind. It is pointed out that the quiet day cosmic ray density in interplanetary space increases the speed of sound beyond the orbit of Earth, reaching 102 km/sec at 50 a.u. if the solar wind should extend that far. Energetic particles from the sun have an effect which may be much larger. The abundance of heavy ions in the solar wind may be significantly below the solar abundance because of diffusion in the solar corona." @default.
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- W2010847057 date "1962-08-01" @default.
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- W2010847057 title "Kinetic properties of interplanetary matter" @default.
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- W2010847057 doi "https://doi.org/10.1016/0032-0633(62)90050-8" @default.
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