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