activity
20072017
most citedANTARES -- A Numerical Tool for Astrophysical RESearch -- With applications to solar granulation

74 citations · 339 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2017★ 6 cited

Structure of the solar photosphere studied from the radiation hydrodynamics code ANTARES

P. Leitner, B. Lemmerer, A. Hanslmeier +4

The ANTARES radiation hydrodynamics code is capable of simulating the solar granulation in detail unequaled by direct observation. We introduce a state-of-the-art numerical tool to…

astro-ph.SR2016★ 11 cited

Dynamics of small-scale convective motions

Birgit Lemmerer, Arnold Hanslmeier, Herbert Muthsam +1

Previous studies have discovered a population of small granules with diameters less than 800 km showing differing physical properties. High resolution simulations and observations…

astro-ph.SR2016

Multidimensional modelling of classical pulsating stars

Herbert J. Muthsam, Friedrich Kupka

After an overview of general aspects of modelling the pulsation- convection interaction we present reasons why such simulations (in multidimensions) are needed but, at the same tim…

astro-ph.SR2015★ 22 cited

Multidimensional realistic modelling of Cepheid-like variables-II: Analysis of a Cepheid model

Eva Mundprecht, Herbert J. Muthsam, Friedrich Kupka

Non-local, time-dependent convection models have been used to explain the location of double-mode pulsations in Cepheids in the HR diagram as well as the existence and location of…

physics.comp-ph2014★ 5 cited

Achievable Efficiency of Numerical Methods for Simulations of Solar Surface Convection

Hannes Grimm-Strele, Friedrich Kupka, Herbert J. Muthsam

We investigate the achievable efficiency of both the time and the space discretisation methods used in Antares for mixed parabolic-hyperbolic problems. We show that the fifth order…

physics.comp-ph2013★ 12 cited

Curvilinear Grids for WENO Methods in Astrophysical Simulations

Hannes Grimm-Strele, Friedrich Kupka, Herbert J. Muthsam

We investigate the applicability of curvilinear grids in the context of astrophysical simulations and WENO schemes. With the non-smooth mapping functions from Calhoun et al. (2008)…