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- W2010059913 abstract "The initial dispersion of a meteor trail which consists of atoms, ions, etc., evaporated from a hot meteoric body has an important bearing on its detectability via electromagnetic wave scattering. In the contemporary literature, the classical diffusion equation, in one form or another, is often used for an approximate description. This leads to much uncertainty and conceptual difficulty. From the Maxwell-Boltzmann viewpoint of kinetic theory, it is found that a new relation in the form of the telegraph equation can be derived which removes the present difficulties and gives closer agreement with observations." @default.
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- W2010059913 date "1970-01-01" @default.
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- W2010059913 title "Fluid Mechanics of Meteor Trails" @default.
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- W2010059913 doi "https://doi.org/10.1063/1.1692803" @default.
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