The role of ocean circulation in driving hemispheric symmetry breaking of the ice shell of Enceladus
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics
Reference67 articles.
1. Dynamics of the global meridional ice flow of Europa's icy shell;Ashkenazy;Nat. Astron.,2018
2. The obliquity of Enceladus;Baland;Icarus,2016
3. Impact of tidal heating on the onset of convection in Enceladus's ice shell;Běhounková;Icarus,2013
4. Tidally-induced melting events as the origin of South-pole activity on Enceladus;Behounkova;Icarus,2012
5. Spatial patterns of tidal heating;Beuthe;Icarus,2013
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1. The role of subsurface ocean dynamics and phase transitions in forming the topography of icy moons;Icarus;2024-04
2. The Effect of Salinity on Ocean Circulation and Ice–Ocean Interaction on Enceladus;The Planetary Science Journal;2024-01-01
3. New global topography of Enceladus: Hypsometry, basins, spherical harmonics, shell thickness, and true polar wander revisited;Icarus;2024-01
4. The modulation effect of ice thickness variations on convection in icy ocean worlds;Monthly Notices of the Royal Astronomical Society;2023-09-02
5. Salt Distribution from Freezing Intrusions in Ice Shells on Ocean Worlds: Application to Europa;The Planetary Science Journal;2023-09-01
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