Solution of the non-LTE problem for molecular gas in planetary atmospheres: superiority of accelerated lambda iteration
- 31 August 1998
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 60 (2), 199-220
- https://doi.org/10.1016/s0022-4073(97)00167-2
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Lower-thermospheric infra-red emissions from minor species during high-latitude twilight—B. Analysis of 15 μm emission and comparison with non-LTE modelsJournal of Atmospheric and Terrestrial Physics, 1994
- A non‐local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 2. Daytime populations of vibrational levelsJournal of Geophysical Research, 1994
- A non‐local thermodynamic equilibrium radiative transfer model for infrared emissions in the atmosphere of Mars: 1. Theoretical basis and nighttime populations of vibrational levelsJournal of Geophysical Research, 1994
- CO2 non‐local thermodynamic equilibrium radiative excitation and infrared dayglow at 4.3 μm: Application to Spectral Infrared Rocket Experiment dataJournal of Geophysical Research: Atmospheres, 1994
- CIRRIS 1A observation of13C16O and12C18O fundamental band radiance in the upper atmosphereGeophysical Research Letters, 1993
- A non-LTE radiative transfer model for infrared bands in the middle atmosphere. II. CO2 (2.7 and 4.3 μm) and water vapour (6.3 μm) bands and N2(1) and O2(1) vibrational levelsJournal of Atmospheric and Terrestrial Physics, 1986
- A non-LTE radiative transfer model for infrared bands in the middle atmosphere. I. Theoretical basis and application to CO2 15 μm bandsJournal of Atmospheric and Terrestrial Physics, 1986
- An Hermitian method for the solution of radiative transfer problemsJournal of Quantitative Spectroscopy and Radiative Transfer, 1976
- Source-Function Equality in MultipletsThe Astrophysical Journal, 1966
- Thermal radiation in the upper atmosphereProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1956