324 citations · 850 across the 6 of their papers we have counts for
6 papers
Intensity contrast from MHD simulations and from HINODE observations
N. Afram, Y. C. Unruh, S. K. Solanki +3
Changes in the solar surface area covered by small-scale magnetic elements are thought to cause long-term changes in the solar spectral irradiance, which are important for determin…
Sub-surface convection zones in hot massive stars and their observable consequences
M. Cantiello, N. Langer, I. Brott +6
We study the convection zones in the outer envelope of hot massive stars which are caused by opacity peaks associated with iron and helium ionization. We determine the occurrence a…
On the origin of microturbulence in hot stars
M. Cantiello, N. Langer, I. Brott +5
We present results from the first extensive study of convection zones in the envelopes of hot massive stars, which are caused by opacity peaks associated with iron and helium ioniz…
Strong horizontal photospheric magnetic field in a surface dynamo simulation
M Schuessler, A. Voegler
Observations with the Hinode spectro-polarimeter have revealed strong horizontal internetwork magnetic fields in the quiet solar photosphere. We aim at interpreting the observation…
Stokes diagnostics of simulated solar magneto-convection
S. Shelyag, M. Schuessler, S. K. Solanki +1
We present results of synthetic spectro-polarimetric diagnostics of radiative MHD simulations of solar surface convection with magnetic fields. Stokes profiles of Zeeman-sensitive…
A solar surface dynamo
A. Voegler, M. Schuessler
Context: Observations indicate that the `quiet' solar photosphere outside active regions contains considerable amounts of magnetic energy and magnetic flux, with mixed polarity on…