Interpretation of high resolution spectra of Mars—II calculations of CO2 abundance, rotational temperature and surface pressure
- 29 July 1971
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 11 (7) , 1075-1086
- https://doi.org/10.1016/0022-4073(71)90127-0
Abstract
No abstract availableKeywords
This publication has 5 references indexed in Scilit:
- Interpretation of high-resolution spectra of Venus: II. The (102-000)II Band of 12C16O18O at 1.71 micronsIcarus, 1970
- Interpretation of high-resolution spectra of Mars I. CO2 abundance and surface pressure derived from the curve of growthIcarus, 1969
- High Dispersion Spectroscopic Observation of Venus IV: The Weak Carbon Dioxide Band at 7883 AApplied Optics, 1969
- Relative intensity calculations for carbon dioxide—IV: Calculations of the partition function for isotopes of CO2Journal of Quantitative Spectroscopy and Radiative Transfer, 1969
- Estimation of rotational line widths of carbon dioxide bandsJournal of Quantitative Spectroscopy and Radiative Transfer, 1969