EGU25-6693, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-6693
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 10:45–12:30 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X2, X2.99
Regionally-triggered geomagnetic reversals
Filipe Terra-Nova and Hagay Amit
Filipe Terra-Nova and Hagay Amit
  • Université de Nantes, LPG UMR 6112, Nantes, France (filipeterranova@gmail.com)

Systematic studies of numerical dynamo simulations reveal that the transition from dipole-dominated non-reversing fields to models that exhibit reversals occurs when inertial effects become strong enough. However, the inertial force is expected to play a secondary role in the force balance in Earth’s outer core. Here we show that reversals in numerical dynamo models with heterogeneous outer boundary heat flux inferred from lower mantle seismic anomalies appear when the amplitude of heat flux heterogeneity is increased. The reversals are triggered at regions of large heat flux in which strong small-scale inertial forces are produced, while elsewhere inertial forces are substantially smaller. When the amplitude of heat flux heterogeneity is further increased so that in some regions sub-adiabatic conditions are reached, regional skin effects suppress small-scale magnetic fields and the tendency to reverse decreases. Our results reconcile the need for inertia for reversals with the theoretical expectation that the inertial force remains secondary in the force balance. Moreover, our results highlight a non-trivial non-monotonic behavior of the geodynamo in response to changes in the amplitude of the core-mantle boundary heat flux heterogeneity.

How to cite: Terra-Nova, F. and Amit, H.: Regionally-triggered geomagnetic reversals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6693, https://doi.org/10.5194/egusphere-egu25-6693, 2025.