The 12- to 20-micron spectrum of Venus: Implications for temperature and cloud structure
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference37 articles.
1. Jupiter's spectrum between 12 and 24 micrometers;Aumann;Science,1976
2. A general relaxation method for inverse solution of the full radiative transfer equation;Chahine;J. Atmos. Sci.,1972
3. Vertical resolution of temperature profiles obtained from remote radiation measurements;Conrath;J. Atmos. Sci.,1972
4. Simultaneous ultraviolet (0.36 μm) and infrared (8 to 20 μm) imaging of Venus: Properties of clouds in the upper atmosphere;Diner,1978
5. The natural atmosphere of Venus as studied with the Mariner 5 radio occultation experiments;Fjeldbo;Astron. J.,1971
Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Measurements of the mean, solar-fixed temperature and cloud structure of the middle atmosphere of Venus;Quarterly Journal of the Royal Meteorological Society;1983-01
2. Airborne spectroscopy and spacecraft radiometry of Venus in the far infrared;Icarus;1982-02
3. Venus;Weather and Climate on Planets;1982
4. 44. Astronomy From Space;Transactions of the International Astronomical Union;1982
5. Commission de L’Astronomie a Partir de L’Espace;Reports on Astronomy;1982
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