Observations of Venus water vapor over the disk of Venus: The 1972–1974 data using the H2O lines at 8197 Å and 8176 Å
- 30 June 1975
- Vol. 25 (2), 268-281
- https://doi.org/10.1016/0019-1035(75)90023-8
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- Comparison of Simultaneous CO2and H2O Observations of VenusJournal of the Atmospheric Sciences, 1975
- Theoretical interpretation of the 0.7820 μm CO2 band and 0.8226 μm H2O line on VenusIcarus, 1975
- Water vapor in Venus determined by airborne observations of the 8200 Å bandIcarus, 1974
- An Expanded Theoretical Interpretation of the Venus 1.05-MICRON co, Line and the Venus 0.8226-MICRON h, O LineThe Astrophysical Journal, 1973
- Does spectroscopic evidence require two scattering layers in the Venus atmosphere?Journal of Quantitative Spectroscopy and Radiative Transfer, 1973
- Water vapor in the atmosphere of VenusIcarus, 1972
- Formation of spectral lines in a planetary atmosphere—II. Spectroscopic evidence for the structure of the visible Venus cloudsJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- The strengths of H2O lines in the 8200 Å region and their application to high dispersion spectra of MarsIcarus, 1971
- A table of the equivalent widths of isolated lines with combined Doppler and collision broadened profilesJournal of Quantitative Spectroscopy and Radiative Transfer, 1968
- Water Vapor on Venus-A Dissent and a ClarificationThe Astrophysical Journal, 1967