Triana, Santiago AndrésReference Systems and Planetology, Royal Observatory of Belgium, Brussels, Belgium
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Trinh, AntonyLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
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Rekier, JérémyReference Systems and Planetology, Royal Observatory of Belgium, Brussels, Belgium
Author
Zhu, PingReference Systems and Planetology, Royal Observatory of Belgium, Brussels, Belgium
Author
Dehant, VéroniqueUCLouvain
Author
Abstract
The cause for the damping of the Earth's free core nutation (FCN) and the free inner core nutation eigenmodes has been a matter of debate since the earliest reliable estimations from nutation observations were made available. Numerical studies are difficult given the extreme values of some of the parameters associated with the Earth's fluid outer core, where important energy dissipation mechanisms can take place. We present a fully 3D numerical model for the FCN capable of describing accurately viscous and Ohmic dissipation processes taking place in the bulk of the fluid core as well as in the boundary layers. We find an asymptotic regime, appropriate for Earth's parameters, where viscous and Ohmic processes contribute to the total damping, with the dissipation taking place almost exclusively in the boundary layers. By matching the observed nutational damping, we infer an enhanced effective viscosity matching and validating methods from previous studies. We suggest that turbulence caused by the Earth's precession can be a source for the enhanced viscosity.
Triana, S. A., Trinh, A., Rekier, J., Zhu, P., & Dehant, V. (2021). The Viscous and Ohmic Damping of the Earth’s Free Core Nutation. Journal of Geophysical Research: Solid Earth, 126(4), 14. https://doi.org/10.1029/2020jb021042 (Original work published 2021)