Formation of spectral lines in planetary atmosphere IV. Theoretical evidence for structure of the jovian clouds from spectroscopic observations of methane and hydrogen quadrupole lines
- 30 April 1973
- Vol. 18 (4) , 637-648
- https://doi.org/10.1016/0019-1035(73)90067-5
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- Formation of spectral lines in planetary atmospheres—I. Theory for cloudy atmospheres; Application to VenusJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- Comments on the Infrared Absorption Line Formation in Cloudy Planetary AtmospheresJournal of the Atmospheric Sciences, 1971
- Recomputation of the absorption strengths of the methane 3v3J-manifolds at 9050 cm-1Journal of Quantitative Spectroscopy and Radiative Transfer, 1971
- Collision-Narrowed Curves of Growth for H2Applied to New Photoelectric Observations of JupiterJournal of the Atmospheric Sciences, 1969
- The Thermal Structure of the Javian AtmosphereJournal of the Atmospheric Sciences, 1969
- A Two-Layer Model of the Jovian CloudsJournal of the Atmospheric Sciences, 1969
- The 2.8-14-MICRON Spectrum of JupiterThe Astrophysical Journal, 1969
- Combined Doppler and Collision Broadening*Journal of the Optical Society of America, 1968
- Simultaneous Effect of Doppler and Foreign Gas Broadening on Spectral LinesPhysical Review B, 1961
- The Effect of Collisions upon the Doppler Width of Spectral LinesPhysical Review B, 1953