Astrophysical radiation magnetohydrodynamics: Applications
Thomas J. Bogdan
NCAR/UCAR

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:	Mercredi, le 10 octobre 2018
Heure:	13:30
Lieu:	Université de Montréal
	Pavillon Roger-Gaudry, Local D-460
Contact:	Paul Charbonneau