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Dynamics and Evolution of SO2 Gas Condensation Around Prometheus-like Volcanic Plumes on Io as Seen by the Near Infrared Mapping SpectrometerNear Infrared Mapping Spectrometer data acquired during the I24, 25, and 27 Io's Fly-bys by Galileo are analyzed to map the SO2 frost abundance and granularity. This allows a better understanding of the dynamics and evolution of gas condensation around volcanic plumes. Additional information is contained in the original extended abstract.
Document ID
20010044817
Document Type
Conference Paper
Authors
Doute, S.
(Centre National de la Recherche Scientifique Grenoble, France)
Lopes-Gautier, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Smythe, W. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Kamp, L. W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Carlson, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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