Surface brightness of a cometary dust tail. I - The calculation technique

Physics

Scientific paper

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Brightness Distribution, Comet Tails, Interplanetary Dust, Surface Properties, Axisymmetric Flow, Comet Nuclei, Particle Motion

Scientific paper

A method for calculating the theoretical brightness distribution in a
cometary dust tail is described for axisymmetric outflow of dust from
the nucleus. The procedure is worked out for a type II tail.

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