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Line positions and intensities of the phosphine (PH) Pentad near 4.5 μm

Abstract:

In order to improve the spectroscopic database for remote sensing of the giant planets, line positions and intensities are determined for the five bands (2ν, ν + ν, 2ν, ν and ν) that comprise the Pentad of PH between 1950 and 2450 cm. Knowledge of PH spectral line parameters in this region is important for the exploration of dynamics and chemistry on Saturn, (using existing Cassini/VIMS observations) and future near-IR data of Jupiter from Juno and ESA's Jupiter Icy Moons Explorer (JUICE). F...

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Publisher copy:
10.1016/j.jms.2014.01.013

Authors


Malathy Devi, V More by this author
Benner, DC More by this author
Kleiner, I More by this author
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Journal:
Journal of Molecular Spectroscopy
Volume:
298
Pages:
11-23
Publication date:
2014-04-05
DOI:
EISSN:
1096-083X
ISSN:
0022-2852
URN:
uuid:a9982e67-1da9-4a02-9564-8cebb73bdc54
Source identifiers:
458114
Local pid:
pubs:458114

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