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Conclusions We perform extensive numerical simulations of 3D rupture propagation governed by the linear slip-weakening in order to define the optimal parameters.
Lg3420362048
Convective Dynamos and the Minimum X-ray Flux in Solar-Type Main Sequence Stars D. J. Bercik 1, G. H. Fisher 1, C. M. Johns-Krull 2, & W. P. Abbett 1 1.
Motivation
Modeling Active Region Magnetic Fields on the Sun
Three-dimensional Modelling of Tunnel Excavation and Lining
M. Ali Etaati CASA-Day April 24 th 2008
AL 6061-T6 - Elastomer Impact Simulations
Www.nanocmos.ac.uk Meeting the Design Challenges of Nano-CMOS Electronics Asen Asenov (PI), Richard Sinnott (eSDirector), all partners e-Science Pilot.
Convective Dynamos and the Minimum X-ray Flux in Solar-Type Main Sequence Stars