High spectral resolution ground-based observations of Venus in the 450- to 1250-cm−1 region
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference23 articles.
1. Celestial infrared calibration sources in the 8–14 micrometer region: Venus and Jupiter;Cecil;AFCRL-TR-73-0559,1973
2. The neutral atmosphere of Venus as studied with the Mariner 5 radio occultation experiment;Fjeldbo;Astron. J.,1971
3. Absolute spectrum of Venus from 2.8 to 14 microns;Gillet;J. Atmos. Sci.,1968
4. Preliminary results of Venus observations between 8 and 13 microns;Hanel;J. Atmos. Sci.,1968
5. A double beam interferometer for the middle infrared;Hanel;Appl. Optics,1969
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1. Intensities and broadening coefficients for the Q branch of the 4v2↔v1 + v2 (471.511 cm-1) band of CO2;Journal of Quantitative Spectroscopy and Radiative Transfer;1993-08
2. Venus spacecraft infrared radiance spectra and some aspects of their interpretation;Applied Optics;1986-05-15
3. Remote sensing by IR heterodyne spectroscopy;Applied Optics;1983-09-01
4. Evidence for high-altitude haze thickening on the dark side of Venus from 10-micron heterodyne spectroscopy of CO2;Icarus;1982-01
5. Venus;Weather and Climate on Planets;1982
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