Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....50..287c&link_type=abstract
Astronomy and Astrophysics, vol. 50, no. 2, July 1976, p. 287-292.
Astronomy and Astrophysics
Astrophysics
8
Ammonia, Infrared Spectra, Jupiter Atmosphere, Planetary Temperature, Atmospheric Models, Planetary Radiation, Temperature Inversions
Scientific paper
A new spectrum of Jupiter at 1.6 per cm resolution in the NH3-nu 2 band spectral range is reported and compared with different synthetic spectra. It is shown that such a comparison cannot lead to a unique temperature profile. It is concluded that the saturation of NH3 is a reasonable assumption. If the adiabatic lapse rate is assumed in the lower atmosphere, atmospheric profiles, showing a strong temperature inversion located at 0.1 atm or deeper, give the best agreement with observations. Some additional absorption features could be due to PH3.
Berezne J.
Combes Michel
Encrenaz Th.
Vapillon Loic
Zeau Y.
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