Models of neutral cometary atmospheres for the interpretation of spectroscopic observations

Details Models of neutral cometary atmospheres for the interpretation of spectroscopic observations Models of neutral cometary atmospheres for the interpretation of spectroscopic observations

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..625t&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, July-Aug. 1985, p. 625-633. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Astronomical Spectroscopy, Cometary Atmospheres, Molecular Collisions, Neutral Gases, Comet Nuclei, Monte Carlo Method

Scientific paper

Various models of neutral cometary atmospheres are compared. It is shown that Haser's formula can be applied to primary molecules. The collision sphere is taken into account in models of secondary molecules, and a model for the neighborhood of the nucleus is examined. Models analogous to those for secondary molecules with allowance for the collision sphere are used for tertiary molecules. Consideration is also given to the Monte Carlo model, and it is noted that this is the only model that can be used in the nonspherically symmetric case.

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