Ground‐based near‐infrared observations of the Venus nightside: The thermal structure and water abundance near the surface
- 25 February 1996
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 101 (E2) , 4595-4622
- https://doi.org/10.1029/95je03567
Abstract
No abstract availableKeywords
This publication has 53 references indexed in Scilit:
- Ground‐based near‐infrared observations of the Venus nightside: 1.27‐μm O2(a1Δg) airglow from the upper atmosphereJournal of Geophysical Research, 1996
- The infrared spectrum of H2S from 1 to 5 μmCanadian Journal of Physics, 1994
- Implications of the high D/H ratio for the sources of water in Venus' atmosphereNature, 1993
- Radiative-transfer models of the night side of VenusIcarus, 1990
- The dark side of VenusIcarus, 1987
- Net thermal radiation in the atmosphere of VenusIcarus, 1985
- A new interpretation of the Venera 11 spectra of VenusIcarus, 1984
- Optimized computation of the voigt and complex probability functionsJournal of Quantitative Spectroscopy and Radiative Transfer, 1982
- Structure of the Atmosphere of Venus up to 110 Kilometers: Preliminary Results from the Four Pioneer Venus Entry ProbesScience, 1979
- Absorption of Infrared Radiant Energy by CO_2 and H_2O IV Shapes of Collision-Broadened CO_2 Lines*Journal of the Optical Society of America, 1969