GENERAL RELATIVISTIC MHD SIMULATIONS OF BLACK HOLE ACCRETION with: Kris Beckwith, Jean-Pierre De Villiers, John Hawley, Shigenobu Hirose, Scott Noble,
GENERAL RELATIVISTIC MHD SIMULATIONS OF BLACK HOLE ACCRETION
SLIDE SHOW 3 B changes due to transport + diffusion III -- * * magnetic Reynold number INDUCTION EQUATION B moves with plasma / diffuses through it.
SHINE SEP Campaign Events: Long-term development of solar corona in build-up to the SEP events of 21 April 2002 and 24 August 2002 A. J. Coyner, D. Alexander,
Thomas Zurbuchen University of Michigan [email protected] The Structure and Sources of the Solar Wind during the Solar Cycle.
Aurora Borealis Northern Lights Assembled by Ken Mitchell Livermore TOPScience.
