Engineering topics
Publications and source records attributed to Gray, L. D..
Venus upper atmosphere average rotational temperature determined from high dispersion spectroscopic observations of 7883 A carbon dioxide band
Relative intensities of lines in vibration and rotation bands of isotopic carbon dioxide in planet Venus, tabulating partition functions
Spectroscopic observations of Venus atmosphere rotational temperature based on carbon dioxide band at 7883 A
Carbon dioxide band in Venus spectrum by dispersion analysis, deriving rotational temperature
Venus carbon dioxide spectral band analysis methods, discussing spectral lines and rotational temperatures obtained
Scientific questions and experimental design for planetary exploration of Jupiter, Mars, Mercury, and Venus
Upper limits to surface pressure and carbon dioxide abundance of Venus atmosphere from combination of mechanical and atmospheric models
High dispersion spectroscopic studies of Venus, discussing spectrograms of one micron carbon dioxide bands, rotational temperatures and reflecting model of atmosphere
Venusian atmosphere cloud top carbon dioxide concentration from Venus 4 probe data
Mechanical and microwave model atmospheres to obtain Venus surface pressure and temperature distribution
Carbon dioxide rotational line intensities relative to integrated intensity of vibration- rotation band tabulated from 160 to 280 degrees K at intervals of 20 degrees K
Upper limit of carbon dioxide abundance in Mercury atmosphere
Inconsistency in Martian surface pressure as calculated by Gray explained, using Leighton and Murray observations
Random Elsasser band model to compute atmospheric transmission of Earth and Mars for 2-micron carbon dioxide bands
Atmospheric radiation calculations emphasizing carbon dioxide and nitrous oxide absorption spectrum, spectral energy distribution, quasi-statistical band model, etc
Spectral absorption due to parallel bands of nitrous oxide computed for temperatures of 200 and 300 degrees K
Spectral emissivity calculations for parallel bands of carbon dioxide at 4.3 microns between 150-600 degrees K, comparing experimental measurements with theoretical calculations
Internal and vibrational partition functions of carbon dioxide and rotational line intensities arising from transitions from ground and first excited states