Angular Momentum Transport in Magnetized Stellar Radiative Zones. IV. Ferraro’s Theorem and the Solar Tachocline
- 10 July 1999
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 519 (2) , 911-917
- https://doi.org/10.1086/307389
Abstract
No abstract availableThis publication has 16 references indexed in Scilit:
- The Rotation of the Solar Core Inferred by Genetic Forward ModelingThe Astrophysical Journal, 1998
- Joint Instability of Latitudinal Differential Rotation and Toroidal Magnetic Fields below the Solar Convection ZoneThe Astrophysical Journal, 1997
- Seismology of the base of the solar convection zoneMonthly Notices of the Royal Astronomical Society, 1997
- Stellar models with microscopic diffusion and rotational mixing. 1: Application to the SunThe Astrophysical Journal, 1995
- Angular Momentum Transport in Magnetized Stellar Radiative Zones. II. The Solar Spin-downThe Astrophysical Journal, 1993
- Inferring the sun's internal angular velocity from observed p-mode frequency splittingsThe Astrophysical Journal, 1989
- On the spin-up of an electrically conducting fluid Part 1. The unsteady hydromagnetic Ekman-Hartmann boundary-layer problemJournal of Fluid Mechanics, 1969
- Influence of an Axial Magnetic Field on the Steady Linear Ekman Boundary LayerPhysics of Fluids, 1968
- Influence of Viscosity, Fluid conductivity, and Wall Conductivity in the Magnetohydrodynamic Rayleigh ProblemsPhysics of Fluids, 1962
- The Non-uniform Rotation of the Sun and its Magnetic FieldMonthly Notices of the Royal Astronomical Society, 1937