Cometary atmospheres: Modeling the spatial distribution of observed neutral radicals

Mathematics

Scientific paper

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Cometary Atmospheres, Monte Carlo Method, Particle Trajectories, Spatial Distribution, Cn Emission, Fluorescence, Mathematical Models, Solar Orbits

Scientific paper

The Monte Carlo particle trajectory model for the saptial distribution of cometary radicals was modified to include the heliocentric distance dependence of the parent molecule velocity, and the heliocentric velocity dependence for CN fluorescence and radiation pressure. Available data on the observed spatial distributions of cometary radicals were studied and a preliminary comparison of newly published data from previous studies is discussed.

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