Interpretation of high-resolution spectra of Mars I. CO2 abundance and surface pressure derived from the curve of growth

Author:

Gray Young L.D.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference25 articles.

1. A Study of the Variations in CO2 Abundance and Surface Pressure of Mars;Barker,1969

2. The abundance and temperature of CO2 in the Martian atmosphere;Belton;Astrophys. J.,1966

3. The strengths, widths and shapes of lines in the vibration rotation bands of CO;Benedict;Astrophys. J.,1962

4. Measurement of the abundance of CO2 in the Martian atmosphere;Carleton;Astrophys. J.,1969

5. Connes, P., Connes, J., Benedict, W. S., and Gray, L. D. (1969a). In press.

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1. Pressure sensor for the Mars 2020 Perseverance rover;Planetary and Space Science;2023-12

2. Fourier transform spectroscopy and the exploration of the solar system;Microchimica Acta;1987-01

3. THE EVOLUTION OF H2O AND CO2 ON EARTH AND MARS;Comparative Planetology;1978

4. Determination of the temperature of the Martian atmosphere;Journal of Quantitative Spectroscopy and Radiative Transfer;1975-07

5. Are the clouds of venus sulfuric acid?;Icarus;1973-04

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