There is evidence for 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) , 465-466
- https://doi.org/10.1016/0022-4073(73)90008-3
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Does spectroscopic evidence require two scattering layers in the Venus atmosphere?Journal of Quantitative Spectroscopy and Radiative Transfer, 1973
- High resolution spectra of Venus—A reviewIcarus, 1972
- Formation of spectral lines in planetary atmospheres—III. The use of analytic scattering diagrams in computations of synthetic spectra for cloudy atmospheresJournal of Quantitative Spectroscopy and Radiative Transfer, 1972
- Spectrum of Venus with a Double-Cloud ModelThe Astrophysical Journal, 1972
- 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 of the upper clouds of VenusReviews of Geophysics, 1972
- The Neutral Atmosphere of Venus as Studied with the Mariner V Radio Occultation ExperimentsThe Astronomical Journal, 1971
- Absorption-Line Formation in a Scattering Planetary Atmosphere: a Test of Van de Hulst's Similarity RelationsThe Astrophysical Journal, 1969
- Composition and Structure of the Clouds of VenusThe Astrophysical Journal, 1968