activity
20072013
most citedSimulations of stellar convection with CO5BOLD

405 citations · 566 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2013★ 51 cited

Progress in Modeling Very Low Mass Stars, Brown Dwarfs, and Planetary Mass Objects

F. Allard, D. Homeier, B. Freytag +2

We review recent advancements in modeling the stellar to substellar transition. The revised molecular opacities, solar oxygen abundances and cloud models allow to reproduce the pho…

astro-ph.SR2011★ 405 cited

Simulations of stellar convection with CO5BOLD

Bernd Freytag, Matthias Steffen, Hans-Günter Ludwig +3

High-resolution images of the solar surface show a granulation pattern of hot rising and cooler downward-sinking material -- the top of the deep-reaching solar convection zone. Con…

astro-ph.SR2009★ 3 cited

The Horizontal Magnetic Field of the Quiet Sun: Numerical Simulations in Comparison to Observations with Hinode

O. Steiner, R. Rezaei, R. Schlichenmaier +2

Three-dimensional magnetohydrodynamic simulations of the surface layers of the Sun intrinsically produce a predominantly horizontal magnetic field in the photosphere. This is a rob…

astro-ph2008★ 1 cited

Supergranulation Scale Connection Simulations

R. F. Stein, A. Nordlund, D. Georgobiani +2

Results of realistic simulations of solar surface convection on the scale of supergranules (96 Mm wide by 20 Mm deep) are presented. The simulations cover only 10% of the geometric…

astro-ph2008★ 88 cited

The horizontal internetwork magnetic field: numerical simulations in comparison to observations with Hinode

O. Steiner, R. Rezaei, W. Schaffenberger +1

Observations with the Hinode space observatory led to the discovery of predominantly horizontal magnetic fields in the photosphere of the quiet internetwork region. Here we investi…

astro-ph2007★ 18 cited

First local helioseismic experiments with CO5BOLD

O. Steiner, G. Vigeesh, L. Krieger +3

With numerical experiments we explore the feasibility of using high frequency waves for probing the magnetic fields in the photosphere and the chromosphere of the Sun. We track a p…