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Positions and Intensities in the 3v2/v2+v4 Vibrational System of 14NH3 Near 4 micron metersAmmonia 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.
Document ID
20060037095
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kleiner, I.
Tarrago, G.
Brown, L. R.
Date Acquired
August 23, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Journal of Molecular Spectroscopy
Subject Category
Atomic And Molecular Physics
Distribution Limits
Public
Copyright
Other
Keywords
ammonia Jupiter Saturn spectroscopy planetary gasses

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