Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982vrsp....2..717m&link_type=abstract
In its Vibrational-Rotational Spectry. for Planetary Atmospheres, Vol. 2 p 717-742 (SEE N82-26134 16-91)
Physics
8
Cometary Atmospheres, Comets, Infrared Spectra, Molecular Spectra, Electron Transitions, Emission Spectra, Rotational Spectra, Spectral Signatures, Spectrum Analysis
Scientific paper
No infrared vibration-rotation spectra have yet been seen for any comet, even though molecular emission features in the ultraviolet and visual regions are common, and gaseous matter is the dominant constituent of the coma. This is in part due to instrumental and atmospheric limitations, but also because non-LTE conditions prevail nearly everywhere throughout the coma and tails, leading to unusual spectra. Aspects of cometary physics and non-LTE spectroscopy are considered. Some aspects of the infrared signatures of cometary molecules are predicted.
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