Dynamic regimes in planetary cores: {\tau}-{\ell} diagrams
Henri-Claude Nataf, Nathana\"el Schaeffer

TL;DR
This paper introduces a novel { au}-{ extlangle}ell{ extrangle} diagram approach to analyze planetary core dynamics, integrating spatial and temporal scales to better understand magnetic field generation, flow organization, and force balances.
Contribution
It presents a comprehensive method using { au}-{ extlangle}ell{ extrangle} diagrams to visualize and analyze planetary core dynamics, linking physical phenomena with scale-dependent time scales.
Findings
Highlights the role of convective power in core dynamics.
Derives a { au}-{ extlangle}ell{ extrangle} translation for force balance.
Provides a toolbox for constructing and interpreting { au}-{ extlangle}ell{ extrangle} diagrams.
Abstract
Planetary cores are the seat of rich and complex fluid dynamics, in which the effects of rotation and magnetic field combine. The equilibria governing the strength of the magnetic field produced by the dynamo effect, the organisation and amplitude of the flow, and those of the density field, remain debated despite remarkable progress made in their numerical simulation. This paper proposes a new approach based on the explicit consideration of the variation of time scales {\tau} with spatial scales {\ell} for the different physical phenomena involved. The {\tau}-{\ell} diagrams thus constructed constitute a very complete graphic summary of the dynamics of the object under study. We highlight the role of the available convective power in controlling this dynamics, together with the relevant force balance, for which we derive a very telling {\tau}-{\ell} translation. Several scenarios are…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Geology and Paleoclimatology Research
