Physics
Scientist
Earth and Planetary Sciences, UC Santa Cruz, Santa Cruz, CA, USA;
Department of Earth and Planetary Sciences, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 and Planetary Sciences, UC Santa Cruz, Santa Cruz, CA, USA
Earth and Planetary Sciences, University of California, Santa Cruz, CA, USA
Comparison of numerical and analytical models of obliquity-driven flows in icy satellite oceans
Implications From Ithaca Chasma for the Thermal and Orbital History of Tethys
Numerical simulations of magnetic field induction in the tidally driven oceans of Europa and Titan (Invited)
Obliquity tides do not significantly heat Enceladus
The response of subsurface oceans in icy satellites to tidally driven forcing
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