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Infrared polarization measurements of Io in 1986New polarization measurements of Io were made with two different polarimeters at 3.8 and 4.8 microns. The measurements, at phase angles of about 2 deg, detect the polarization of reflected sunlight at both wavelengths. Only upper limits can be determined for the volcanic activity in 1986, but these limits show that there has been a remarkable decrease in activity, particularly of the Loki volcano, at these short wavelengths. The 1984 data (Goguen and Sinton (1985) are reanalyzed with the new model, which includes polarization of reflected sunlight. The large amount of thermal emission from the Loki volcano in 1984 produced a polarization that was dominant over that of reflected sunlight.
Document ID
19880064321
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sinton, William M.
(Hawaii, University Honolulu, United States)
Goguen, Jay D.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Nagata, Tetsuya
(Hawaii, University Honolulu; Kyoto University Japan, United States)
Ellis, H. Benton, Jr.
(Texas, University Austin, United States)
Werner, Michael
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1988
Publication Information
Publication: Astronomical Journal
Volume: 96
ISSN: 0004-6256
Subject Category
Lunar And Planetary Exploration
Accession Number
88A51548
Funding Number(s)
CONTRACT_GRANT: NCA2-34
CONTRACT_GRANT: NGL-12-057-001
Distribution Limits
Public
Copyright
Other

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