Revised Molecular Line Parameters of Ammonia
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line parameters Ammonia Revised Molecular HITRAN G↗
Engineering topics
Cottaz, C.
Publications and source records attributed to Cottaz, C..
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↗