Dynamo constraints on the long-term evolution of Earth's magnetic field strength - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Geophysical Journal International Year : 2021

Dynamo constraints on the long-term evolution of Earth's magnetic field strength

Christopher J. Davies
  • Function : Author
Richard K. Bono
  • Function : Author
Domenico G. Meduri
  • Function : Author
Julien Aubert
Samuel Greenwood
  • Function : Author
Andrew J. Biggin
  • Function : Author


Elucidating the processes in the liquid core that have produced observed paleointensity changes over the last 3.5 Gyrs is crucial for understanding the dynamics and long-term evolution of Earth's deep interior. We combine numerical geodynamo simulations with theoretical scaling laws to investigate the variation of Earth's magnetic field strength over geological time. Our approach follows the study of Aubert et al. (2009), adapted to include recent advances in numerical simulations, mineral physics and paleomagnetism. We first compare the field strength within the dynamo region and on the core-mantle boundary (CMB) between a suite of 314 dynamo simulations and two power-based theoretical scaling laws. The scaling laws are both based on a Quasi-Geostropic (QG) force balance at leading-order and a Magnetic, Archimedian, and Coriolis (MAC) balance at first order and differ in treating the characteristic lengthscale of the convection as fixed (QG-MAC-fixed) or determined as part of the solution (QG-MAC-free). When the dataset is filtered to retain only simulations with magnetic to kinetic energy ratios greater than at least two we find that the internal field together with the RMS and dipole CMB fields exhibit power-law behaviour that is compatible with both scalings within uncertainties arising from different heating modes and boundary conditions. However, while the extrapolated intensity based on the QG-MAC-free scaling matches Earth's modern CMB field, the QG-MAC-fixed prediction shoots too high and also significantly overestimates paleointensities over the last 3.5 Gyrs. We combine the QG-MAC-free scaling with outputs from 275 realisations of core-mantle thermal evolution to construct synthetic true dipole moment (TDM) curves spanning the last 3.5 Gyrs. Best-fitting TDMs reproduce binned PINT data during the Bruhnes and before inner core nucleation within observational uncertainties, but PINT does not contain the predicted strong increase and subsequent high TDMs during the early stages of inner core growth. The best-fit models are obtained for a present-day CMB heat flow of 11-16 TW, increasing to 17-22 TW at 4 Ga, and predict a minimum TDM at inner core nucleation.
Fichier principal
Vignette du fichier
ggab342.pdf (2.37 Mo) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03590027 , version 1 (26-02-2022)





Christopher J. Davies, Richard K. Bono, Domenico G. Meduri, Julien Aubert, Samuel Greenwood, et al.. Dynamo constraints on the long-term evolution of Earth's magnetic field strength. Geophysical Journal International, 2021, pp.2355-2377. ⟨10.1093/gji/ggab342⟩. ⟨insu-03590027⟩
7 View
16 Download



Gmail Facebook Twitter LinkedIn More