Does spectroscopic evidence require two scattering layers in the Venus atmosphere?
- 31 May 1973
- journal article
- research article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 13 (5), 461-463
- https://doi.org/10.1016/0022-4073(73)90007-1
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
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- Discrete space theory of radiative transfer II. Stability and non-negativityProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1969
- Discrete space theory of radiative transfer I. FundamentalsProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1969
- Absorption-Line Formation in a Scattering Planetary Atmosphere: a Test of Van de Hulst's Similarity RelationsThe Astrophysical Journal, 1969
- The Phase Curve of Venus and the Nature of its CloudsJournal of the Atmospheric Sciences, 1968
- Rotational Temperature and Phase Variation of the Carbon Dioxide Bands of Venus.The Astrophysical Journal, 1956