Compaction-driven convection in the growing inner core: research letter

The Earth's inner core (IC) is known to exhibit heterogeneous structures with their origins still unknown. From the onset of nucleation, the IC can grow via sedimentation and compaction of iron crystals freezing out from the fluid outer core. Previous studies of IC growth have shown entrapment...

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Bibliographic Details
Main Authors: Lim, Kang Wei (Author) , Deguen, R. (Author) , Cébron, D. (Author) , Schulze, Amelie (Author) , Mandea, Mioara (Author)
Format: Article (Journal)
Language:English
Published: 16 December 2024
In: Geophysical research letters
Year: 2024, Volume: 51, Issue: 23, Pages: 1-12
ISSN:1944-8007
DOI:10.1029/2024GL110749
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1029/2024GL110749
Verlag, kostenfrei, Volltext: https://onlinelibrary.wiley.com/doi/abs/10.1029/2024GL110749
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Author Notes:K.W. Lim, R. Deguen, D. Cébron, A. Schulze, and M. Mandea
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Summary:The Earth's inner core (IC) is known to exhibit heterogeneous structures with their origins still unknown. From the onset of nucleation, the IC can grow via sedimentation and compaction of iron crystals freezing out from the fluid outer core. Previous studies of IC growth have shown entrapment of fluid within the solid matrix, and unstable density profiles in 1D can appear depending on the efficiency of fluid percolation. In this study, we perform simulations of IC growth in spherical geometries (assuming axisymmetry). We find that it is possible for the IC to develop large-scale convective flows under certain conditions and, in some instances, produce small-scale heterogeneites close to the IC boundary. Assuming representative values for the physical properties of the Earth's IC, we show that it is possible for the IC to exhibit compaction-driven convection today.
Item Description:Online verfügbar: 03. Dezember 2024
Gesehen am 10.07.2025
Physical Description:Online Resource
ISSN:1944-8007
DOI:10.1029/2024GL110749