'Hall mhd' diaporamas de présentation

Fast Magnetic Reconnection: Bridging Laboratory and Space Plasma Physics

Fast Magnetic Reconnection: Bridging Laboratory and Space Plasma Physics. Bhattacharjee, W. Fox, K. Germaschewski , a nd Y-M. Huang Center for Integrated Computation and Analysis of Reconnection and Turbulence (CICART ) Center for Magnetic Self-Organization (CMSO)

863 views • 64 slides

Multi-scale Computational Challenge

A New Methodology for Multi-scale Simulation of Plasmas Self-Adaptive Simulations Computational Group at SciberQuest, Inc. in collaboration with Georgia Tech Supported by NSF ITR Grant. Multi-scale Computational Challenge. Large disparity in spatial and temporal scales

525 views • 38 slides

Alex Lazarian

3D Reconnection of Weakly Stochastic Magnetic Field and its Implications. Alex Lazarian. Astronomy Department and Center for Magnetic Self-Organization in Astrophysical and Laboratory Plasmas. Collaboration: Ethan Vishniac, Grzegorz Kowal and Otminowska-Mazur.

447 views • 31 slides

Comparison of the Martian and Venusian Wakes Fedorov, CESR, Toulouse

311 views • 20 slides

Kinetic Effects on the Linear and Nonlinear Stability Properties of Field-Reversed Configurations

2003 APS DPP Meeting, October 2003. Kinetic Effects on the Linear and Nonlinear Stability Properties of Field-Reversed Configurations. E. V. Belova PPPL. In collaboration with : R. C. Davidson, H. Ji, M. Yamada ( PPPL ). OUTLINE:. I. Linear stability (n=1 tilt mode, prolate FRCs)

317 views • 20 slides

Prandtl number dependence of magnetic-to-kinetic dissipation

Prandtl number dependence of magnetic-to-kinetic dissipation. What gets in, will get out Even for vanishing viscosity What if magnetic fields contribute?. Axel Brandenburg (Nordita ?? CU Boulder ). (ApJ 791, 12 (2014). Finite dissipation at vanishing viscosity.

181 views • 17 slides