NASA NTRS · 20000080628
Modeling Io's Heat Flow: Constraints from Galileo PPR Data
Abstract
We 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.
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Rathbun, J. A., Spencer, J. R., Tamppari, L. K.. 2000-03-01. Modeling Io's Heat Flow: Constraints from Galileo PPR Data. https://ntrs.nasa.gov/citations/20000080628
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