The kinematics of hexagonal magnetoconvection

DOI10.1080/03091928308209061zbMath0537.76092OpenAlexW2060650579WikidataQ114640607 ScholiaQ114640607MaRDI QIDQ3323573

M. R. E. Proctor, D. J. Galloway

Publication date: 1983

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

Full work available at URL: https://doi.org/10.1080/03091928308209061

zbMATH Keywords

modal analysisthree dimensionalmagnetic Reynolds numbersolar granulationHexagonal magnetoconvectionmagnetic transport equationSpiral field linestesselation cells between two planes

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Diffusion and convection (76R99) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (4)

Solar cycle modelling using spatiotemporal decomposition schemes ⋮ Mean advection effects in turbulence ⋮ Small-scale magnetic buoyancy and magnetic pumping effects in a turbulent convection ⋮ Reflections on magnetoconvection

Cites Work

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• Kinematical Hydromagnetic Theory and its Application to the Low Solar Photosphere.
• Axisymmetric convection in the presence of a magnetic field
• The rate of magnetic field penetration through a Bénard convection layer
• Convection in an imposed magnetic field. Part 1. The development of nonlinear convection
• Convection in an imposed magnetic field. Part 2. The dynamical regime
• Nonlinear interaction of magnetic field and convection
• On the dynamic interaction between magnetic fields and convection
• Magnetic flux ropes and convection
• Topological pumping of magnetic flux by three-dimensional convection
• NOTE ON THE VIBRATION OF MEMBRANES

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