The Solar Tachocline


Tachocline

Enhancement and suppression of turbulence by energetic-particle-driven geodesic acoustic modes. Evolution of lithium abundance in the Sun and solar twins. An experiment for testing general relativity in the inner solar system. The Astrophysical Journal, Vol. Rossby waves in the magnetic fluid dynamics of a rotating plasma in the shallow-water approximation. Journal of Experimental and Theoretical Physics, Vol. Shear flow instabilities in shallow-water magnetohydrodynamics.

The Solar Tachocline

Journal of Fluid Mechanics, Vol. Eddy, drift wave and zonal flow dynamics in a linear magnetized plasma. Durston, Sam and Gilbert, Andrew D. Transport and instability in driven two-dimensional magnetohydrodynamic flows. Effects ofq-profile structures on intrinsic torque reversals. Formation of a chemical-composition gradient beneath the convection zone and the early evolution of the sun.

1. INTRODUCTION

Physical Review Letters, Vol. Caleo, Andrea Balbus, Steven A. Differential rotation and radiative equilibrium in the Sun: Cambridge University Press Online publication date: August Print publication year: Export citation Recommend to librarian Recommend this book.

The Solar Dynamo: Plasma Flows

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Submission history

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  • The importance of the solar tachocline - ScienceDirect.
  • A Self-consistent Model of the Solar Tachocline - IOPscience.
  • Through the Necromanteum: Project Far-Reach.
  • A Self-consistent Model of the Solar Tachocline;
  • Träume im Mondschein (JULIA 23) (German Edition)!

We present a local but fully nonlinear model of the solar tachocline, using three-dimensional direct numerical simulations. The tachocline forms naturally as a statistically steady balance between Coriolis, pressure, buoyancy, and Lorentz forces beneath a turbulent convection zone.

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Uniform rotation is maintained in the radiation zone by a primordial magnetic field, which is confined by meridional flows in the tachocline and convection zone. Such balanced dynamics has previously been found in idealized laminar models, but never in fully self-consistent numerical simulations. The computer you are using is not registered by an institution with a subscription to this article. Please log in below. Find out more about journal subscriptions at your site. If you would like to buy this article, but not online, please contact custserv iop.