Wednesday, January 17, 2018
Peter Gilman presents results from an analytical model for magnetic buoyancy and rotational instabilities in a full spherical shell tachocline that includes rotation. differential rotation close to that observed helioseismicly, and toroidal field.
Submitted by whawkins on July 25, 2016 - 4:38pm
Peter Gilman is a Senior Scientist Emeritus in the High Altitude Observatory at NCAR specializing in the fluid dynamics and magneto-fluid dynamics of the Sun and stars. His current interest focuses on the hydrodynamics and magneto hydrodynamics of the solar tachocline.