Rotational relaxation of the 0001 level of CO2 including radiative transfer in the 4.3-μm band of planetary atmospheres
- 31 August 1985
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 34 (2) , 101-114
- https://doi.org/10.1016/0022-4073(85)90037-8
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- The non-equilibrium rotational distribution function of an emitting gasChemical Physics Letters, 1983
- Modeling of the 10-μm natural laser emission from the mesospheres of Mars and VenusIcarus, 1983
- Infrared energy levels and intensities of carbon dioxide—IIJournal of Quantitative Spectroscopy and Radiative Transfer, 1981
- Pressure broadening of the dipole and Raman lines of CO2 by He and Ar. Temperature dependenceThe Journal of Chemical Physics, 1979
- Classical trajectory studies of rotational transitions in Ar–CO2 collisionsThe Journal of Chemical Physics, 1977
- Infrared Radiative Emission in the Venusian MesosphereJournal of the Atmospheric Sciences, 1976
- Infrared Radiative Heating and Cooling in the Venusian Mesosphere.I: Global Mean Radiative EquilibriumJournal of the Atmospheric Sciences, 1972
- Broadening of Infrared Absorption Lines at Reduced Temperatures: Carbon Dioxide†Journal of the Optical Society of America, 1972
- A modified Feautrier methodJournal of Quantitative Spectroscopy and Radiative Transfer, 1971
- Classical Theory of Rotational Relaxation in Diatomic GasesThe Journal of Chemical Physics, 1970