EGU25-19659, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-19659
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 29 Apr, 09:25–09:35 (CEST)
 
Room K1
The influence of a stably stratified layer on the Earth's outer core waves.
Fleur Seuren1,2, Santiago Triana1, Jérémy Rekier1, Véronique Dehant1, and Tim Van Hoolst1,2
Fleur Seuren et al.
  • 1Royal Observatory of Belgium, Reference Systems and Planetology, Belgium (fleur.seuren@ksb-orb.be)
  • 2KU Leuven, Institute of Astronomy, Belgium

Seismic studies, mineral physics, thermal evolution models and geomagnetic observations offer conflicting evidence about the presence of a stably stratified layer at the top of the Earth's fluid outer core. Such a convectively stable layer could have a strong influence on the Earth's hydromagnetic waves, propagating underneath the core-mantle boundary (CMB) that are used to probe the outermost region of the core. Here we present numerical solutions for the eigenmodes in a neutrally stratified sphere permeated by a magnetic field with and without a top stable layer, allowing for fluid exchanges between the stable layer and the neutrally stratified bulk of the core and angular momentum exchanges across the CMB through viscous- and electromagnetic coupling. On interannual time-scales, we find torsional Alfvén waves that are only marginally affected by weak to moderate stratification strength in the outer layer. At decadal time-scales similarly weak stable layers promote the appearance of waves, that propagate primarily within the stable layer itself and resemble Magneto-Archimedes-Coriolis (MAC) waves, even though they interact with the adiabatic fluid core below.

How to cite: Seuren, F., Triana, S., Rekier, J., Dehant, V., and Van Hoolst, T.: The influence of a stably stratified layer on the Earth's outer core waves., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19659, https://doi.org/10.5194/egusphere-egu25-19659, 2025.