Three-dimensional kinematic dynamos dominated by strong differential rotation
From MaRDI portal
Publication:4892853
DOI10.1017/S0022112096001292zbMath0864.76098MaRDI QIDQ4892853
Publication date: 24 June 1997
Published in: Journal of Fluid Mechanics (Search for Journal in Brave)
convectionboundary effectsrotating spheremeridional circulationsEarth's coreboundary zonesoscillatory and quadrupolar fieldssteady dipolar solutions
Related Items
Planar velocity dynamos in a sphere ⋮ Finite-amplitude convection in rotating spherical fluid shells ⋮ Dynamo theory then and now ⋮ Three-Dimensional Dynamo Waves In a Sphere ⋮ Kinematic dynamo action in a sphere: Effects of periodic time-dependent flows on solutions with axial dipole symmetry ⋮ Numerical modeling of magnetohydrodynamic convection in a rapidly rotating spherical shell: Weak and strong field dynamo action ⋮ On a dynamo driven by topographic precession ⋮ Eulerian and Lagrangian means in rotating, magnetohydrodynamic flows II. Braginsky’s nearly axisymmetric dynamo
Cites Work