By E. Reister, M. Müller, K. Binder (auth.), Prof. Dr. Egon Krause, Prof. Dr. Willi Jäger (eds.)
The ebook summarizes the result of the initiatives of the excessive functionality Computing heart Stuttgart (HLRS) for the yr 2000. the main major contributions were chosen in a systematic assessment procedure. jointly they supply an summary of contemporary advancements in excessive functionality computing and simulation. Reflecting the shut cooperation of the HLRS with undefined, designated emphasis has been wear the economic relevance of the awarded effects and techniques. The e-book as a result turns into a set of showcases for an cutting edge blend of the cutting-edge modeling, novel numerical algorithms and using innovative excessive functionality computing platforms.
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Extra resources for High Performance Computing in Science and Engineering 2000: Transactions of the High Performance Computing Center Stuttgart (HLRS) 2000
Earth Plan. Int. : Recent developments in the dynamo theory of planetary magnetism. Ann. Rev. Earth Plan Sci. : Convection-Driven Zonal Flows in the Major Planets. : The onset of thermal convection in a rotating cylindrical annulus in the presence of a magnetic field. Phys. Earth Plan. Int. : On convection driven dynamos in rotating spherical shells. Studia geoph. et geod. : "Hydrodynamic and Hydromagnetic Stability". : Numerical Modeling of the Geodynamo: A Systematic Parameter Study. Geophys.
As a source we choose a simple, relatively broadband (2 - 8 Hz) wavelet with the main frequency centered at 5 Hz. This is similar to the average frequency content of the high-frequency Pn phase as it is observed along some prominent refraction seismic profiles . 3 The teleseismic Pn To test a hypothesis of an upper mantle scattering waveguide, we carried out finite-difference based numerical simulations of wave propagation for a set of 2-dimensional models with randomly distributed velocity fluctuations in the Earth upper mantle.
At the surface r = (ri + ro)/2 for the same instances of time. Solid (dashed) lines indicate positive (negative) values. t"" 20 E. H. 8 Fig. 2. Energies of convection as a function of time t in the case T = 104 , P = l. 106 (from top to bottom). The energy Ep is several orders of magnitude smaller than the other ones and has not been plotted for this reason. figure the time dependence has already experienced a doubling of the period at this point as is evident from the time series of the kinetic energies plotted in figure 2.