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H2 and HD Spectroscopic StatusHD spectra was studied in the UV about as thoroughly as those of H2. The vibration-rotation line positions are known. However, the theory does not do well in calculating the absorption strengths. These tend to be stronger than the quadrupole strengths for H2 and so more lines were measured. The state of knowledge of the HD line positions of vibration-rotation constants is summarized. The HD absorption strength measurements are also summarized. A summary of absorption strengths for HD is tabulated.
Document ID
19820018259
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Margolis, J. S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Vibrational-Rotational Spectry. for Planetary Atmospheres, Vol. 2
Subject Category
Lunar And Planetary Exploration
Accession Number
82N26135
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19820018258Collected WorksVibrational-Rotational Spectroscopy for Planetary Atmospheres, volume 2
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