Revised Molecular Line Parameters of Ammonia
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line parameters Ammonia Revised Molecular HITRAN G↗
Engineering topics
Tarrago, G.
Publications and source records attributed to Tarrago, G..
Line Positions and Intensities in the 2v(sub 2)/v(sub 4)Vibrational System of (sup 14)NH(sub 3) near 5-7 meu m
Ammonia is the fourth most abundant constituent in the atmosphere of Jupiter, after hydrogen, helium and methane.
ammonia intensities infrared spectroscopy↗
Positions, Intensities and Self-Broadened Line Widths of the 3(sub v2)-(sub v2) And (sub v2) + (sub v4)-(sub v2)Hot Bands of (sub 14)NH(sub 3) In the 5 to 8 mue Region
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Ammonia spectroscopy infrared intensities widths↗
Positions and Intensities in the 2v4/v1/v3 Vibrational System of 14NH3 near 3 mu m
Line positions and line intensities of the v1, v3 and 2V4 bands of 14NH3 were analyzed using line positions from 0.0054 cm-1 apodized resolution FT spectra recorded at Orsay and using line intensities from 0.011 cm-1 unapodized resolution FT spectra recorded at Kitt peak National Observatory. The theoretical model and the set of programs developed for treating the infrared system v1/v3/2v4 of ammonia are briefly discussed.
ammonia Jupiter infrared mapping↗
Methyl Chloride V5 Region Line Shape Parameters and Rotational Constants for the V2, V5 and 2V3 Vibrational Band
Methyl chloride (CH3Cl) is relatively abundant in the Earth's atmosphere, and because it is easily photodissociated is an important source of the chlorine atoms which are involved in the destruction of atmospheric ozone.
methyl chloride rotational constants vibrational b↗
Positions and Intensities in the 3v2/v2+v4 Vibrational System of 14NH3 Near 4 micron meters
Ammonia is the fourth most abundant constituent in the atmospheres of Jupiter and Saturn, after hydrogen, helium and methane. This relative abundance is attested by the presence in the infrared planetary spectra of many absorption features observed in the range of fundamental bands and also in the higher bands. Reported are experimental line positions and intensities of selected ammonia bands.
ammonia Jupiter Saturn spectroscopy planetary gass↗
Analysis of 3v(sub 2) and v(sub 2)+v(sub 4) of (sup 14)NH(sub 3) Near 4 Microns
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remote sensing Fourier transform spectrometer FTS ↗
Methane and its isotopes - Current status and prospects for improvement
Numerous changes made for the 1991 and 1992 versions of the HITRAN database in the 0-6185/cm region for molecular line parameters of methane are described. An assessment of deficiencies in the parameters is presented.
Brown, L. R.↗
Recent high resolution laboratory determinations of line broadening and intensity parameters: PH3, CH3D, and CO2
Recent unpublished laboratory work on rovibrational line strengths and broadening coefficients which is of interest in the study of planetary atmospheres was reviewed. The molecules discussed are PH3, CH3D and CO2.
Suarez, C. B.↗