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Numerical Dynamo Simulations Reproduce Paleomagnetic Field Behavior
Author(s) -
Meduri D. G.,
Biggin A. J.,
Davies C. J.,
Bono R. K.,
Sprain C. J.,
Wicht J.
Publication year - 2021
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2020gl090544
Subject(s) - paleomagnetism , dynamo theory , geology , dynamo , geophysics , earth's magnetic field , convection , field (mathematics) , range (aeronautics) , dipole , geodesy , mechanics , magnetic field , physics , materials science , mathematics , quantum mechanics , pure mathematics , composite material
Numerical geodynamo simulations capture several features of the spatial and temporal geomagnetic field variability on historical and Holocene timescales. However, a recent analysis questioned the ability of these numerical models to comply with long‐term paleomagnetic field behavior. Analyzing a suite of 50 geodynamo models, we present here the first numerical simulations known to reproduce the salient aspects of the paleosecular variation and time‐averaged field behavior since 10 Ma. We find that the simulated field characteristics covary with the relative dipole field strength at the core‐mantle boundary (dipolarity). Only models dominantly driven by compositional convection, with an Ekman number (ratio of viscous to Coriolis forces) lower than 10 −3 and a dipolarity in the range 0.34–0.56 can capture the observed paleomagnetic field behavior. This dipolarity range agrees well with state‐of‐the‐art statistical field models and represents a testable prediction for next generation global paleomagnetic field model reconstructions.