The 800-1200 inverse centimeter absorption spectrum of Jupiter

Details The 800-1200 inverse centimeter absorption spectrum of Jupiter The 800-1200 inverse centimeter absorption spectrum of Jupiter

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207.1002r&link_type=abstract

Astrophysical Journal, vol. 207, Aug. 1, 1976, pt. 1, p. 1002-1006.

Astronomy and Astrophysics

Astrophysics

24

Absorption Spectra, Abundance, Atmospheric Temperature, Jupiter Atmosphere, Thermal Emission, Ammonia, Astronomical Models, Brightness Temperature, Computer Techniques, Infrared Spectra, Telluric Lines, Temperature Profiles

Scientific paper

Synthetic spectra computed from radiative models of the Jovian thermal
structure are compared with observed spectra. The results imply a
subsaturated NH3 abundance near the temperature minimum, and an
additional opacity source near 1100 kaysers. Evidence is found for the
presence of PH3 consistent with a solar P abundance.

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