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20082026
most citedThe horizontal internetwork magnetic field: numerical simulations in comparison to observations with Hinode

88 citations · 219 across the 8 of their papers we have counts for

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astro-ph.SR2026

Kilogauss magnetic fields from simulations of small-scale dynamo action in the convective envelope of a white dwarf

Fabio Riva, Tim Cunningham, Hans-Günter Ludwig +2

About 20% of white dwarfs are observed to host large-scale magnetic fields, but the origin of white dwarf magnetism remains uncertain. Small-scale turbulent dynamos (SSDs), which e…

astro-ph.SR2020★ 5 cited

On the influence of magnetic topology on the propagation of internal gravity waves in the solar atmosphere

G. Vigeesh, M. Roth, O. Steiner +1

The solar surface is a continuous source of internal gravity waves (IGWs). IGWs are believed to supply the bulk of the wave energy for the lower solar atmosphere, but their existen…

astro-ph.SR2020★ 12 cited

Interaction of magnetic fields with a vortex tube at solar subgranular scale

C. E. Fischer, G. Vigeesh, P. Lindner +3

Using high-resolution spectropolarimetric data recorded with the Swedish 1 m Solar Telescope, we have identified several instances of granular lanes traveling into granules. These…

astro-ph.SR2015★ 80 cited

On The Evolution of Magnetic White Dwarfs

P. -E. Tremblay, G. Fontaine, B. Freytag +5

We present the first radiation magnetohydrodynamics simulations of the atmosphere of white dwarf stars. We demonstrate that convective energy transfer is seriously impeded by magne…

astro-ph.SR2012★ 22 cited

Three-dimensional magnetohydrodynamic simulations of M-dwarf chromospheres

S. Wedemeyer, H. -G. Ludwig, O. Steiner

We present first results from three-dimensional radiation magnetohydrodynamic simulations of M-type dwarf stars with CO5BOLD. The local models include the top of the convection zon…

astro-ph.SR2010

Numerical simulations of wave propagation in the solar chromosphere

C. Nutto, O. Steiner, M. Roth

We present two-dimensional simulations of wave propagation in a realistic, non-stationary model of the solar atmosphere. This model shows a granular velocity field and magnetic flu…