Variation of Jupiter's CH4 and NH3 bands with position on the planetary disk
- 31 January 1974
- Vol. 21 (1), 47-54
- https://doi.org/10.1016/0019-1035(74)90090-6
Abstract
No abstract availableKeywords
This publication has 4 references indexed in Scilit:
- Formation of spectral lines in planetary atmosphere IV. Theoretical evidence for structure of the jovian clouds from spectroscopic observations of methane and hydrogen quadrupole linesIcarus, 1973
- A Two-Layer Model of the Jovian CloudsJournal of the Atmospheric Sciences, 1969
- Molecular Absorption and the Possible Structure of the Cloud Layers of Jupiter and SaturnJournal of the Atmospheric Sciences, 1969
- Atmospheric Composition of the Jovian PlanetsJournal of the Atmospheric Sciences, 1969