The Jovian temperature structure obtained by inversion of infrared spectral measurements

Details The Jovian temperature structure obtained by inversion of infrared spectral measurements The Jovian temperature structure obtained by inversion of infrared spectral measurements

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...38..342w&link_type=abstract

Icarus, vol. 38, June 1979, p. 342-348.

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Atmospheric Temperature, Infrared Spectra, Jupiter Atmosphere, Planetary Atmospheres, Temperature Profiles, Atmospheric Models, Error Analysis, Radiative Transfer, Stratosphere, Temperature Measurement, Jupiter, Temperatures, Thermal Structure, Infrared, Spectrum, Pioneer 10, Radio Occultation, Inversion, Stratosphere, Radiation, Transport, Heating, Observations, Models, Equilibrium, Pioneer 11

Scientific paper

The results of inversions of infrared spectral measurements indicate that there exist temperature structures in the region of the temperature minimum at about 0.1 bar which are significantly different from radiative models. It is demonstrated that this difference can be accounted for in terms of errors in the retrieved temperature structures caused by the lack of observations which adequately define the thermal structure in the lower stratosphere.

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