Some Key Issues in Solar Plasmas (Leiden, March 21, 2005) Eric Priest.
OUR AMAZING SUN (Alexandria, March 26, 2006) Eric Priest.
Turbulent Convection in the Laboratory
HAO 07/20141 Double cycles and instabilities in EULAG- MHD simulations of solar convection Paul Charbonneau Département de Physique, Université de Montréal.
Mega-grants for environmental challenges 24-26.05.2012
SLIDE SHOW 3 B changes due to transport + diffusion III -- * * magnetic Reynold number INDUCTION EQUATION B moves with plasma / diffuses through it.
An update on convection zone modeling with the ASH code
Heating the Corona and Driving the Solar Wind
Some Key Issues in Solar Plasmas
Coronal Dynamics - Can we detect MHD shocks and waves by Solar B ? K. Shibata Kwasan Observatory Kyoto University 2003 Feb. 3-5 Solar B Meeting @ ISAS.
Plumes in turbulent convection
ASTEROSEISMOLOGY CoRoT session, January 13, 2007 Jadwiga Daszyńska-Daszkiewicz Instytut Astronomiczny, Uniwersytet Wrocławski.