Hostname: page-component-848d4c4894-8bljj Total loading time: 0 Render date: 2024-06-20T18:00:19.937Z Has data issue: false hasContentIssue false
  • English
  • Français

High spectral resolution interferometric planetary observations in the 7–25 μ region

Published online by Cambridge University Press:  14 August 2015

R. A. Hanel ,
V. G. Kunde ,
T. Meilleur  and
G. Stambach
R. A. Hanel
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.
V. G. Kunde
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.
T. Meilleur
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.
G. Stambach
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The thermal emission spectra of Venus, Mars, Jupiter, and the moon were observed at the coude focus of the McDonald Observatory 107-inch telescope in the 400–1400 cm−1 spectral range with spectral resolutions of 0.3–0.7 cm−1. A preliminary interpretation of the Venus/lunar ratio spectrum allows identification of four upper state CO2 bands in the Venusian atmosphere at 791, 828, 865, and 961 cm−1 and confirms previous observations of the broad absorption-like depression around 890 cm−1. The rotational structure of the 791 and 961 cm−1 bands is well developed at this spectral resolution.

Type
Part I: Venus
Information
Symposium - International Astronomical Union , Volume 40: Planetary Atmospheres , 1971 , pp. 44 - 47
Copyright
Copyright © Reidel 1971 

References

Gillett, F. C., Low, F. J., and Stein, W. A.: 1968, J. Atmospheric Sci. 25, 594.2.0.CO;2>CrossRefGoogle Scholar
Hanel, R. A., Forman, M., Stambach, G., and Meilleur, T.: 1968, J. Atmospheric Sci. 25, 586.2.0.CO;2>CrossRefGoogle Scholar
Hanel, R. A., Forman, M., Meilleur, T., Wescott, R., and Pritchard, J.: 1969, J. Appl. Opt. 8, 2059.CrossRefGoogle Scholar
Sinton, W. M. and Strong, J.: 1960, Astrophys. J. 131, 470.CrossRefGoogle Scholar