I. Temperatures of polar ice deposits on mercury and the moon. II. Jovian atmospheric dynamics from Galileo imaging

I. Temperatures of polar ice deposits on mercury and the moon. II. Jovian atmospheric dynamics from Galileo imaging

<p>Locations on Mercury that produce ice-like radar responses lie within impact craters that have very cold, permanently shaded floors. The retention of possible ice deposits is determined largely by their temperature. We present model- calculated temperatures of flat surfaces and surfaces...

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Bibliographic Details
Main Author: Vasavada, Ashwin R.
Format: Others
Language:en
Published: 1998
Online Access:https://thesis.library.caltech.edu/7447/1/Vasavada_ar_1998.pdf
Vasavada, Ashwin R. (1998) I. Temperatures of polar ice deposits on mercury and the moon. II. Jovian atmospheric dynamics from Galileo imaging. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/ps1y-d710. https://resolver.caltech.edu/CaltechTHESIS:01282013-083854060 <https://resolver.caltech.edu/CaltechTHESIS:01282013-083854060>

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https://thesis.library.caltech.edu/7447/1/Vasavada_ar_1998.pdf
Vasavada, Ashwin R. (1998) I. Temperatures of polar ice deposits on mercury and the moon. II. Jovian atmospheric dynamics from Galileo imaging. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/ps1y-d710. https://resolver.caltech.edu/CaltechTHESIS:01282013-083854060 <https://resolver.caltech.edu/CaltechTHESIS:01282013-083854060>

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