Dynamo theory for the interface between the convection zone and the radiative interior of a star: Part I model equations and exact solutions

DOI10.1080/03091928608210092zbMath0624.76044OpenAlexW1977238687WikidataQ114640396 ScholiaQ114640396MaRDI QIDQ3026573

Edward E. Deluca, Peter A. Gilman

Publication date: 1986

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091928608210092

zbMATH Keywords

Coriolis forceexact solutionsdynamomeridional circulationmagnetic field generationsolar convection zonemagnetic induction equationDifferential rotationhelical convectionhomogeneous incompressible fluids

Mathematics Subject Classification ID

Absolute and convective instability and stability in hydrodynamic stability (76E15) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Galactic and stellar dynamics (85A05)

Related Items (2)

Effects of a subadiabatic layer on convection and dynamos in spherical wedge simulations ⋮ Dynamo theory for the interface between the convection zone and the radiative interior of a star part

Cites Work

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• Periodic and aperiodic dynamo waves
• α²-Dynamos and taylor's constraint
• Convection in an imposed magnetic field. Part 1. The development of nonlinear convection
• Convection in an imposed magnetic field. Part 2. The dynamical regime
• The macrodynamics of α-effect dynamos in rotating fluids
• Nonlinear dynamics of boussinesq convection in a deep rotating spherical shell-i
• Numerical solutions of the nonlinear α-effect dynamo equations
• The magneto-hydrodynamics of a rotating fluid and the earth’s dynamo problem

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