Dynamique � grande échelle des disques protoplanétaires
Our results were produced by post-processing both ideal density distributions and sophisticated magnetohydrodynamic (MHD) col- lapse simulations with radiative ...
The Three-Dimensional Structure of Magnetic Reconnection in SSX... 3 Différents modes de propagation d'une onde MHD . . . . . . . . 96. 3.2 Chocs MHD stationnaires transverses . . . . . . . . . . . . . . . . . . . . 97. 3.2.1 ... Magnetohydrodynamic Simulation of Reconnection in Turbulent ...6.16: Cuts through the density field (LHS) and the velocity-field intensity (RHS) in a fully developed Ms = 3 and MA = 1.66 MHD turbulence. High values of the ... Evolution des poussi`eres dans les chocs - HAL ThèsesAs for magnetic circular dichroism, MHD can be observed by inverting the sign of either the orbital momentum or of the magnetization, i.e. by ...
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