Generation of Magnetic Fields in Gravitationally Forming Structures in the Early Universe Russell M. Kulsrud Princeton Plasma Physics Laboratory.
Comparing classical and lab plasma dynamos S. Prager University of Wisconsin useful discussions with D. Craig, H. Ji, J. Sarff, E. Zweibel.
1 Challenge the future 1 1 Structural control method research for MAV application Yao Lu Chairman : Prof. Dr. Fred van Keulen Supervisor: Dr. Hans Goosen,
Astrobiology presentation
Dalton Review (1)
Astrobiology Grant
Solar and Interplanetary Sources of Geomagnetic disturbances Yu.I. Yermolaev, N. S. Nikolaeva, I. G. Lodkina, and M. Yu. Yermolaev Space Research Institute.
Contribution of KIT to LHD Topics from collaboration research on MHD phenomena in LHD S. Masamune, K.Y. Watanabe 1), S. Sakakibara 1), Y. Takemura, KIT.
Strongly interacting matter in an external magnetic field Pavel Buividovich (Regensburg University) DPG Jahrestagung, Dresden, March 4-8, 2013.
Comparing classical and lab plasma dynamos
Generation of Magnetic Fields in Gravitationally Forming Structures in the Early Universe
Modeling of turbulence using filtering, and the absence of ``bottleneck’’ in MHD
