Infrared transmission properties of CO, HCI, and SO2 and their significance for the greenhouse effect on Venus
- 30 September 1969
- Vol. 11 (2), 159-170
- https://doi.org/10.1016/0019-1035(69)90041-4
Abstract
No abstract availableKeywords
This publication has 5 references indexed in Scilit:
- Temperature structure of nongray planetary atmospheresIcarus, 1969
- Carbon monoxide in the Venus atmosphereThe Astrophysical Journal, 1968
- Traces of HCl and HF in the atmosphere of VenusThe Astrophysical Journal, 1967
- Absorption Line Broadening in the InfraredApplied Optics, 1962
- Interferometric Method of Measuring the Spectral Slit Width of Spectrometers*Journal of the Optical Society of America, 1955