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modeling io's heat flow: constraints from galileo ppr dataWe attempt to improve on previous Io heat flow estimates by using higher resolution data from Galileo Photopolarimeter Radiometer (PPR) and improved thermophysical models of the surface, including finite thermal inertia, the pedestal effect, and disk-resolved radiance.
Document ID
20000080628
Document Type
Conference Paper
Authors
Rathbun, J. A.
(Lowell Observatory Flagstaff, AZ United States)
Spencer, J. R.
(Lowell Observatory Flagstaff, AZ United States)
Tamppari, L. K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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