Statistics – Computation
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...408..668c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 408, no. 2, p. 668-677.
Statistics
Computation
30
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.
Bos Brent Jon
Combi Michael R.
Smyth William H.
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