Determination of the instantaneous geostrophic flow within the three-dimensional magnetostrophic regime
From MaRDI portal
Publication:4626264
DOI10.1098/rspa.2018.0412zbMath1407.86013arXiv1806.06612OpenAlexW3098481518WikidataQ92162293 ScholiaQ92162293MaRDI QIDQ4626264
Philip W. Livermore, Colin M. Hardy, Jitse Niesen, Jiawen Luo, Kuan Li
Publication date: 27 February 2019
Published in: Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1806.06612
Related Items (3)
The inherent instability of axisymmetric magnetostrophic dynamo models ⋮ On magnetostrophic dynamos in annular cores ⋮ Self-exciting fluid dynamos
Cites Work
- Unnamed Item
- Unnamed Item
- An optimal Galerkin scheme to solve the kinematic dynamo eigenvalue problem in a full sphere
- Successive elimination of shear layers by a hierarchy of constraints in inviscid spherical-shell flows
- Approaching a realistic force balance in geodynamo simulations
- Evolution of non-linear α 2-dynamos and taylor's constraint
- α2-Dynamos and taylor's constraint
- The structure of Taylor's constraint in three dimensions
- Dynamically consistent magnetic fields produced by differential rotation
- The cross-over to magnetostrophic convection in planetary dynamo systems
- Taylor state dynamos found by optimal control: axisymmetric examples
- αω-Dynamos and Taylor's constraint
- Physical constraints on the coefficients of Fourier expansions in cylindrical coordinates
- The magneto-hydrodynamics of a rotating fluid and the earth’s dynamo problem
- Spherical convective dynamos in the rapidly rotating asymptotic regime
- On the theory of core-mantle coupling
- On the modified Taylor constraint
- On magnetostrophic mean-field solutions of the geodynamo equations
This page was built for publication: Determination of the instantaneous geostrophic flow within the three-dimensional magnetostrophic regime