I. Thermal Evolution of Ganymede and Implications for Surface Features. II. Magnetohydrodynamic Constraints on Deep Zonal Flow in the Giant Planets. III. A Fast Finite-Element Algorithm for Two-Dimensional Photoclinometry

I. Thermal Evolution of Ganymede and Implications for Surface Features. II. Magnetohydrodynamic Constraints on Deep Zonal Flow in the Giant Planets. III. A Fast Finite-Element Algorithm for Two-Dimensional Photoclinometry

<p>The work is divided into three independent papers:</p> <p>PAPER I:</p> <p>Thermal evolution models are presented for Ganymede, assuming a mostly differentiated initial state of a water ocean overlying a rock layer. The only heat sources are assumed to be primor...

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Bibliographic Details
Main Author: Kirk, Randolph Livingstone
Format: Others
Published: 1987
Online Access:https://thesis.library.caltech.edu/4554/1/Kirk_rl_1987.pdf
Kirk, Randolph Livingstone (1987) I. Thermal Evolution of Ganymede and Implications for Surface Features. II. Magnetohydrodynamic Constraints on Deep Zonal Flow in the Giant Planets. III. A Fast Finite-Element Algorithm for Two-Dimensional Photoclinometry. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/T5PT-S948. https://resolver.caltech.edu/CaltechETD:etd-11142006-131417 <https://resolver.caltech.edu/CaltechETD:etd-11142006-131417>

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https://thesis.library.caltech.edu/4554/1/Kirk_rl_1987.pdf
Kirk, Randolph Livingstone (1987) I. Thermal Evolution of Ganymede and Implications for Surface Features. II. Magnetohydrodynamic Constraints on Deep Zonal Flow in the Giant Planets. III. A Fast Finite-Element Algorithm for Two-Dimensional Photoclinometry. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/T5PT-S948. https://resolver.caltech.edu/CaltechETD:etd-11142006-131417 <https://resolver.caltech.edu/CaltechETD:etd-11142006-131417>

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