The OH distribution in cometary atmospheres - A collisional Monte Carlo model for heavy species

Statistics – Computation

Scientific paper

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Cometary Atmospheres, Hydroxyl Radicals, Molecular Collisions, Monte Carlo Method, Velocity Distribution, Exosphere, Halley'S Comet, Heavy Nuclei, Iue, Comets, Comae, Oh Radical, Distribution, Models, Collisions, Kinetics, Monte Carlo Method, Scattering, Parameters, Molecular Processes, Water, Production Rate, Halley, Velocity, Calculations, Satellite Observations, Iue Satellite

Scientific paper

The study presents an extension of the cometary atmosphere Monte Carlo particle trajectory model formalism which makes it both physically correct for heavy species and yet computationally reasonable. The derivation accounts for the collision path and scattering redirection of a heavy radical traveling through a fluid coma with a given radial distribution in outflow speed and temperature. The revised model verifies that the earlier fast-H atom approximations used in earlier work are valid, and it is applied to a case where the heavy radical formalism is necessary: the OH distribution. It is found that a steeper variation of water production rate with heliocentric distance is required for a water coma which is consistent with the velocity-resolved observations of Comet P/Halley.

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