Approximate estimates for the surface pressure of mars based on infrared transmission data in the 2μ region
Author:
Publisher
Elsevier BV
Subject
Spectroscopy,Atomic and Molecular Physics, and Optics,Radiation
Reference6 articles.
1. Transmission of the atmosphere of Mars in the region of 2 μ
2. Infrared spectra of stars and planets—IV. The spectrum of Mars, 1–2·5 μ, and the structure of its atmosphere;Kuiper;Comm. Lunar Planetary Lab.,1964
3. On the Determination of Rotational Line Half‐Widths of Diatomic Molecules
4. The Abundance and Temperature of CO_{2} in the Martian Atmosphere
5. High-Dispersion Spectroscopic Obervations of Mars. I. The CO_{2} Content and Surface Pressure
Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Publications by S. S. Penner;Modern Developments in Energy, Combustion and Spectroscopy;1993
2. High-Resolution Infrared Spectroscopy of Planetary Atmospheres;Molecular Spectroscopy;1972
3. Planetary atmospheres;Eos, Transactions American Geophysical Union;1971
4. Martian Topography from the Mariner 6 and 7 Infrared Spectra;The Astronomical Journal;1970-10
5. Interpretation of high-resolution spectra of Mars I. CO2 abundance and surface pressure derived from the curve of growth;Icarus;1969-11
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