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Magnetic Taylor-Proudman Constraint Explains Flows into the Tangent Cylinder

Alban Pothérat* and Kélig Aujogue

François Debray

  • Coventry University, Centre for Fluid and Complex Systems, Mile Lane, Coventry CV1 2NL, United Kingdom

  • Laboratoire National des Champs Magnétiques Intenses (LNCMI), CNRS UPR 3228, EMFL, Université Toulouse III—Paul Sabatier, Université Fédérale Toulouse Midi-Pyrénées, Institut National des Sciences Appliquées, Université Grenoble Alpes, 38042 Grenoble CEDEX, France

  • *Contact author: alban.potherat@coventry.ac.uk

Disorder, Topology, and Fluid Mechanics: Symmetry Breaking and Mechanical Function in Complex Structures

Yifan Zhang

Symmetry 18 562 (2026)

The Elbert range of magnetostrophic convection. II. Comparing linear theory to nonlinear low- Rm simulations

Susanne Horn and Jonathan M. Aurnou

Proc. R. Soc. A. 481 20240016 (2025)

Seven decades of exploring planetary interiors with rotating convection experiments

Alban Pothérat and Susanne Horn

Comptes Rendus. Physique 25 21 (2025)

How Earth’s Magnetic Field Influences Flows in the Planet’s Core

Rachel Berkowitz

Physics 17 142 (2024)

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