Transmission of CO2 in the atmosphere of Venus for the spectral region near 7 microns |
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Authors: | Louise Gray Young |
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Affiliation: | Department of Astronomy, San Diego State University, San Diego, California 92182, USA |
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Abstract: | The transmission in the 7-μm “window” opf Venus was calculated for a 7-layer model atmosphere. The synthetic spectra show that radiation from the layer 20–30 km above the surface would reach the top of the atmosphere between 6.2 and 7.0 μm if there were no absorption besides the isotopic CO2 bands; for the 7.0- to 8.2-μm region, the radiating level would be located 40–50 km above the surface of Venus. The brightness temperature for the entire region is 430°K; for the above two regions it is 494 and 341°K, respectively. |
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