The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

HG Ludwig, Å Nordlund - arXiv preprint astro-ph/0005319, 2000 - arxiv.org
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …
被引用次数：202 相关文章
[PDF] researchgate.net

[PDF][PDF] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund… - arXiv preprint astro-ph … - researchgate.net
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …

The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund… - ASTRONOMY AND …, 2000 - diva-portal.org
The effects of numerical resolution on hydrodynamical surface convection simulations and spectral
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[PDF] core.ac.uk

[PDF][PDF] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund, RF Stein - Astron. Astrophys, 2000 - core.ac.uk
The computationally demanding nature of radiativehydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …
[PDF] psu.edu

[PDF][PDF] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund, RF Stein - ASTROPHYSICS, 2000 - Citeseer
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …

[引用][C] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund… - ASTRONOMY AND …, 2000 - swepub.kb.se
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The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, AA Nordlund, RF Stein - Astron. Astrophys., 2000 - inspirehep.net
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …
[PDF] academia.edu

[PDF][PDF] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund, RF Stein - arXiv preprint astro-ph … - academia.edu
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …
[PS] msu.edu

[PS][PS] The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, A Nordlund, RF Stein - ASTROPHYSICS, 2000 - pa.msu.edu
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …

The effects of numerical resolution on hydrodynamical surface convection simulations and spectral line formation

M Asplund, HG Ludwig, Å Nordlund… - Astronomy and …, 2000 - ui.adsabs.harvard.edu
The computationally demanding nature of radiative-hydrodynamical simulations of stellar
surface convection warrants an investigation of the sensitivity of the convective structure and …