Parametrized pressure and temperature profiles for Titan

Details Parametrized pressure and temperature profiles for Titan Parametrized pressure and temperature profiles for Titan

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jqsrt..39..485d&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 39, June 1988, p. 485-488.

Computer Science

1

Atmospheric Pressure, Atmospheric Temperature, Pressure Distribution, Satellite Atmospheres, Temperature Profiles, Titan, Parameterization, Radio Occultation, Voyager Project

Scientific paper

Vertical (0-200-km altitude) profiles of temperature and pressure for the Titan atmosphere are calculated on the basis of simplified approximations involving empirical polynomials and exponential functions. The model equations are presented; the determination of the nonzero parameter values employed in the calculations is outlined; and the profiles are compared with the Voyager radio-occultation data compiled by Lindal et al. (1983). Generally good agreement is obtained, except for the temperature values in the altitude range 66-86 km.

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