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Observations of the martian 1.2 μ CO2 bands

Published online by Cambridge University Press:  14 August 2015

Edwin S. Barker
Edwin S. Barker*
Affiliation:
McDonald Observatory, The University of Texas, Fort Davis, Tex., U.S.A.

Abstract

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A method to determine independently the Martian surface pressure from measurements of individual lines in the 1.2030 and 1.2177 μ CO2 bands is presented. Observations obtained during the 1967 apparition and some preliminary results of the 1969 apparition observations yield CO2 abundances near 100 m-atm and surface pressures of 4–8 mb.

Type
Part II: Mars
Information
Symposium - International Astronomical Union , Volume 40: Planetary Atmospheres , 1971 , pp. 191 - 195
Copyright
Copyright © Reidel 1971 

References

Barker, E. S.: 1969, unpublished Ph.D. Dissertation, The University of Texas.Google Scholar