On the interpretation of the “inverse phase effect” for CO2 equivalent widths on Venus
- 26 October 1973
- Vol. 20 (2) , 146-152
- https://doi.org/10.1016/0019-1035(73)90047-x
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Formation of spectral lines in planetary atmospheres—I. Theory for cloudy atmospheres; Application to VenusJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- Formation of spectral lines in a planetary atmosphere—II. Spectroscopic evidence for the structure of the visible Venus cloudsJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- Composition and structure of planetary atmospheresSpace Science Reviews, 1971
- Multiple Scattering of Polarized Light in Planetary Atmospheres Part II. Sunlight Reflected by Terrestrial Water CloudsJournal of the Atmospheric Sciences, 1971
- Clouds of Venus: Evidence for Their NatureScience, 1971
- Multiple Scattering of Polarized Light in Planetary Atmospheres. Part I. The Doubling MethodJournal of the Atmospheric Sciences, 1971
- Interpretation of the Venus CO_{2} Absorption BandsThe Astrophysical Journal, 1970
- Absorption-Line Formation in a Scattering Planetary Atmosphere: a Test of Van de Hulst's Similarity RelationsThe Astrophysical Journal, 1969
- Rotational Temperature and Phase Variation of the Carbon Dioxide Bands of Venus.The Astrophysical Journal, 1956
- Diffuse Reflection by Planetary Atmospheres.The Astrophysical Journal, 1950