On Jovian temperature profiles obtained by inverting thermal spectra

Details On Jovian temperature profiles obtained by inverting thermal spectra On Jovian temperature profiles obtained by inverting thermal spectra

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..760w&link_type=abstract

Astrophysical Journal, vol. 203, Feb. 1, 1976, pt. 1, p. 760-763.

Astronomy and Astrophysics

Astrophysics

10

Infrared Spectra, Jupiter Atmosphere, Methane, Planetary Temperature, Temperature Profiles, Thermal Radiation, Astronomical Models, Atmospheric Models, Atmospheric Temperature, Planetary Radiation, Spectral Bands

Scientific paper

Defects in the inversion of observed thermal infrared spectra of Jupiter
to obtain temperature structures are reviewed. An ambiguity is noted
when the 7.8-micron band of CH 4 is used, and alternative temperature
structures are obtained.

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