Astronomy and Astrophysics Seminars

Seismic imaging of the power spectrum of turbulent convection in the solar interior

by Dr. Shravan Hanasoge (Seismic imaging of the power spectrum of turbulent convection in the solar interior)

Thursday, January 3, 2013 from to (Asia/Kolkata)
at Colaba Campus ( DAA A269 )
Description
A variety of methods are brought to bear on the problem of appreciating
turbulent convection in the solar interior. Seismic analyses of observations taken by
the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory reveal
convective  velocities that are almost two orders in magnitude smaller than current
theoretical and computational predictions. The associated Reynolds' stresses would be too
small to explain meridional circulation and differential rotation in the convection envelope
and throw into question models of dynamo action in the Sun.