How does the solar wind blow? A simple kinetic model

Physics

Scientific paper

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Scientific paper

A simple kinetic model of solar wind ejection is presented. It provides an alternative to the fluid derivation given in most space physics textbooks, and allows one to derive the wind speed from simple principles. This kind of description emphasizes the role of the electrostatic field which is implicit in the fluid point of view. It also illustrates the inadequacy of the classical heat conduction law in space plasmas, and allows one to deal with non-equilibrium velocity distributions, which are ubiquitous there.

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