Astrophysical radiation magnetohydrodynamics: Applications
Thomas J. Bogdan

The theory of radiation magnetohydrodynamics developed in the first lecture will now be applied to astrophysical problems of interest, namely: radiatively driven wind driving and accretion, and turbulent magnetic dynamos including radiative transfer.

Date: Wednesday, 10 October 2018
Time: 13:30
Where: Université de Montréal
  Pavillon Roger-Gaudry, Local D-460
Contact: Paul Charbonneau