Methane absorption in the Jovian atmosphere I. The Lorentz half-width in the 3v3 band at 1.1 μm
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference32 articles.
1. Inhomogeneous models of the atmosphere of Jupiter;Axel;Astrophys. J.,1972
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3. An Observational Test of Absorption Line Formation Models in the Jovian Atmosphere;Bergstralh,1972
4. Recomputation of the absorption strengths of the methane 3v3 J-manifolds at 9050 cm−1;Bergstralh;J. Quant. Spectr. Radiative Transfer,1971
5. Spectrophotometry of the 1.5 μm window of Jupiter;Binder;Astronom. J.,1972
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1. Jupiter's Atmospheric Composition and Cloud Structure Deduced from Absorption Bands in Reflected Sunlight;Journal of the Atmospheric Sciences;1979-07
2. The Jovian spectrum in the region 0.4–1.1 µm: The C/H ratio;Reviews of Geophysics;1978
3. The interpretation of Jovian methane absorptions;The Astrophysical Journal;1977-02
4. Estimates of methane and ammonia abundance in the Jovian atmosphere with allowance for scattering in the clouds;Icarus;1977-01
5. Observations of NH3 in the atmosphere of Jupiter during 1973, 1974;Icarus;1977-01
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