Slide 1 Non-disruptive MHD Dynamics in Inward-shifted LHD Configurations 1.Introduction 2.RMHD simulation 3.DNS of full 3D MHD 4. Summary MIURA, H., ICHIGUCHI, K., NAKAJIMA,…
Halo Current and Resistive Wall Simulations of ITER H.R. Strauss1, Linjin Zheng2, M. Kotschenreuther2, W.Park3, S. Jardin3, J. Breslau3, A.Pletzer3, R. Paccagnella4, L. Sugiyama5,…
The role of the kink instability in magnetically driven jets Dimitrios Giannios Max-Planck Institute for Astrophysics In collaboration with Henk Spruit Structure of the talk…
Attempts to build a dynamo-based predictive tool Magnetic persistence between the current sunspot cycleâs amplitude and previous cycleâs polar fields (Schatten, late 1970âs;…
Non-disruptive MHD Dynamics in Inward-shifted LHD Configurations 1.Introduction 2.RMHD simulation 3.DNS of full 3D MHD 4. Summary MIURA, H., ICHIGUCHI, K., NAKAJIMA, N.,…
Cellular Dynamo in a Rotating Spherical Shell Alexander Getling Lomonosov Moscow State University Moscow, Russia Radostin Simitev, Friedrich Busse University of Bayreuth,…
Observational signature for global evolution of solar magnetic fields From url of D. Hathaway What is a dynamo? A dynamo is a process by which the magnetic field in an electrically…