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Vertical Distribution of PH(sub 3) in Saturn from Observations of the 1-0 and 3-2 Rotational LinesFar-infrared Fourier-transform spectrometer measurements of the 1-0 and 3-2 PH(sub 3) transitions in Saturn's disk near 267 and 800 GHz (8.9 and 26.7 cm(sup -1)), respectively, were analyzed simultaneously to derive a global mean profile for the PH(sub 3) vertical mixing ratio between 100 and 800 mbar total pressure.
Document ID
20060040701
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/17492
Authors
Orton, G.
Serabyn, E.
Lee, Y.
Date Acquired
August 23, 2013
Publication Date
January 1, 1999
Publication Information
Publication: ICARUS
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Other
Keywords
Posphine photochemistry Saturn spectroscopy atmospheres

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