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 |
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