"Topological structure and reconnection of magnetic flux lines are investigated by analyzing the numerical solution of the Boussinesq magneto-hydrodynamic equations in a rotating spherical shell. Five pairs of Taylor-Proudman vortex columns are generated and drift westward steadily. Magnetic field is intensified around the tops of these vortex columns. Magnetic flux lines connect east-west adjacent domains of intense magnetic field, which rnigrate eastward relative to the vortex columns. We describe the variation of topology of magnetic flux lines associated with this eastward migration.
The convection-driven MHD dynamo in a rotating spherical shell is simulated numerically. Convection ...
VK: resolve; Karhunen, J.; ReSoLVEWe report the discovery of an azimuthal dynamo wave of a low-order...
The magnetic field in rapidly rotating dynamos is spatially inhomogeneous. The axial variation of th...
Intensification mechanisms of magnetic field by thermal convection in a rotating spherical shell are...
"The mechanism of generation of magnetic field by thermal convection is investigated by analyzing th...
"A convoluted pattern of streamlines in a steady state of thermal convection of a Boussinesq fluid b...
"A strong axial magnetic dipole field having the magnetic energy 15 times larger than the kinetic of...
Spherical shell dynamo models based on rotating convection show that the flow within the tangent cyl...
Abstract. Numerical calculations of fluid dynamos powered by thermal convection in a rotating, elect...
The problem of the generation of magnetic fields by convection in rotating spherical fluid shells is...
The generation of a magnetic field in numerical simulations of the geodynamo is an intrinsically 3-D...
A convection-driven MHD dynamo in a rotating spherical shell, with clearly defined structural elemen...
Context. Stellar convection zones are characterized by vigorous high-Reynolds number turbulence at l...
Context: Stellar convection zones are characterized byvigorous high-Reynolds number turbulence at lo...
This paper reports 3D numerical simulations of compressible, thermal convection in a small rectil...
The convection-driven MHD dynamo in a rotating spherical shell is simulated numerically. Convection ...
VK: resolve; Karhunen, J.; ReSoLVEWe report the discovery of an azimuthal dynamo wave of a low-order...
The magnetic field in rapidly rotating dynamos is spatially inhomogeneous. The axial variation of th...
Intensification mechanisms of magnetic field by thermal convection in a rotating spherical shell are...
"The mechanism of generation of magnetic field by thermal convection is investigated by analyzing th...
"A convoluted pattern of streamlines in a steady state of thermal convection of a Boussinesq fluid b...
"A strong axial magnetic dipole field having the magnetic energy 15 times larger than the kinetic of...
Spherical shell dynamo models based on rotating convection show that the flow within the tangent cyl...
Abstract. Numerical calculations of fluid dynamos powered by thermal convection in a rotating, elect...
The problem of the generation of magnetic fields by convection in rotating spherical fluid shells is...
The generation of a magnetic field in numerical simulations of the geodynamo is an intrinsically 3-D...
A convection-driven MHD dynamo in a rotating spherical shell, with clearly defined structural elemen...
Context. Stellar convection zones are characterized by vigorous high-Reynolds number turbulence at l...
Context: Stellar convection zones are characterized byvigorous high-Reynolds number turbulence at lo...
This paper reports 3D numerical simulations of compressible, thermal convection in a small rectil...
The convection-driven MHD dynamo in a rotating spherical shell is simulated numerically. Convection ...
VK: resolve; Karhunen, J.; ReSoLVEWe report the discovery of an azimuthal dynamo wave of a low-order...
The magnetic field in rapidly rotating dynamos is spatially inhomogeneous. The axial variation of th...
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