Development of a Line-by-Line and a Correlated <i>k</i>-Distribution Radiation Models for Planetary Atmospheres
Author:
Affiliation:
1. Department of Planetology, Kobe University, Japan
2. Department of Earth Sciences, Okayama University, Japan
3. Department of Cosmosciences, Hokkaido University, Japan
Publisher
Meteorological Society of Japan
Subject
Atmospheric Science
Link
https://www.jstage.jst.go.jp/article/jmsj/101/1/101_2023-003/_pdf
Reference64 articles.
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3. Baranov, Y. I., W. J. Lafferty, and G. T. Fraser, 2004: Infrared spectrum of the continuum and dimer absorption in the vicinity of the O2 vibrational fundamental in O2/CO2 mixtures. J. Mol. Spectrosc., 228, 432-440.
4. Bézard, B., C. de Bergh, D. Crisp, and J.-P. Maillard, 1990: The deep atmosphere of Venus revealed by high-resolution nightside spectra. Nature, 345, 508-511.
5. Bézard, B., A. Fedorova, J.-L. Bertaux, A. Rodin, and O. Korablev, 2011: The 1.10- and 1.18-µm nightside windows of Venus observed by SPICAV-IR aboard Venus Express. Icarus, 216, 173-183.
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