Search Results - "Happenhofer, Natalie"
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Total-variation-diminishing implicit–explicit Runge–Kutta methods for the simulation of double-diffusive convection in astrophysics
Published in Journal of computational physics (01-05-2012)“…We put forward the use of total-variation-diminishing (or more generally, strong stability preserving) implicit–explicit Runge–Kutta methods for the time…”
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Optimized strong stability preserving IMEX Runge–Kutta methods
Published in Journal of computational and applied mathematics (15-12-2014)“…We construct and analyze robust strong stability preserving IMplicit–EXplicit Runge–Kutta (IMEX RK) methods for models of flow with diffusion as they appear in…”
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A low Mach number solver: Enhancing applicability
Published in Journal of computational physics (01-03-2013)“…In astrophysics and meteorology there exist numerous situations where flows exhibit small velocities compared to the sound speed. To overcome the stringent…”
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Total Variation Diminishing Implicit Runge-Kutta Methods for Dissipative Advection-Diffusion Problems in Astrophysics
Published in Proceedings in applied mathematics and mechanics (01-12-2011)“…We investigate the properties of dissipative full discretizations for the equations of motion associated with models of flow and radiative transport inside…”
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Total-Variation-Diminishing Implicit-Explicit Runge-Kutta Methods for the Simulation of Double-Diffusive Convection in Astrophysics
Published 30-12-2011“…Journal of Computational Physics, vol. 231, 3561-3586 (2012) We put forward the use of total-variation-diminishing (or more generally, strong stability…”
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A Low Mach Number Solver: Enhancing Applicability
Published 16-11-2012“…Journal of Computational Physics, vol 236, 96-118 (2013) In astrophysics and meteorology there exist numerous situations where flows exhibit small velocities…”
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Simulations of stellar convection, pulsation and semiconvection
Published 13-09-2010“…We report on modelling in stellar astrophysics with the ANTARES code. First, we describe properties of turbulence in solar granulation as seen in…”
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