Andere Kunden interessierten sich auch für
![Optimum Aerodynamic Design & Parallel Navier-Stokes Computations ECARP ¿ European Computational Aerodynamics Research Project]( "Optimum Aerodynamic Design & Parallel Navier-Stokes Computations ECARP ¿ European Computational Aerodynamics Research Project")
Optimum Aerodynamic Design & Parallel Navier-Stokes Computations ECARP ¿ European Computational Aerodynamics Research Project74,99 €![Computation and Comparison of Efficient Turbulence Models for Aeronautics ¿ European Research Project ETMA]( "Computation and Comparison of Efficient Turbulence Models for Aeronautics ¿ European Research Project ETMA")
Computation and Comparison of Efficient Turbulence Models for Aeronautics ¿ European Research Project ETMA37,99 €![Recent Development of Aerodynamic Design Methodologies]( "Recent Development of Aerodynamic Design Methodologies")
Recent Development of Aerodynamic Design Methodologies37,99 €![Flow Simulation with High-Performance Computers II]( "Flow Simulation with High-Performance Computers II")
Flow Simulation with High-Performance Computers II42,99 €![Elastische Kapseln im hydrodynamischen Fluss]( "Elastische Kapseln im hydrodynamischen Fluss")
Elastische Kapseln im hydrodynamischen Fluss89,00 €![Mathematica for Physicists and Engineers]( "Mathematica for Physicists and Engineers")
Mathematica for Physicists and Engineers59,99 €![Fraktale Aggregate]( "Fraktale Aggregate")
Fraktale Aggregate59,00 €
The mathematical part covers the implementation and
comparison of different numerical schemes to solve
the equations of radiation hydrodynamics. One and the
same two-dimensional model of solar granulation is
simulated with different high resolution numerical
methods (essentially non-oscillatory and convex
non-oscillatory) and non-grey short characteristic
radiative transfer. Furthermore the influence of
artificial diffusivities is studied. The second part
covers two astrophysical applications. A
two-dimensional non-grey high resolution simulation
of a downflowing plume in the sun and a grey
three-dimensional simulation of the quiet sun are
presented.
comparison of different numerical schemes to solve
the equations of radiation hydrodynamics. One and the
same two-dimensional model of solar granulation is
simulated with different high resolution numerical
methods (essentially non-oscillatory and convex
non-oscillatory) and non-grey short characteristic
radiative transfer. Furthermore the influence of
artificial diffusivities is studied. The second part
covers two astrophysical applications. A
two-dimensional non-grey high resolution simulation
of a downflowing plume in the sun and a grey
three-dimensional simulation of the quiet sun are
presented.