242 citations · 792 across the 8 of their papers we have counts for
8 papers
Origin of the hemispheric asymmetry of solar activity
M. Schüssler, R. H. Cameron
The frequency spectrum of the hemispheric asymmetry of solar activity shows enhanced power for the period ranges around 8.5 years and between 30 and 50 years. This can be understoo…
Solar Dynamics, Rotation, Convection and Overshoot
S. Hanasoge, M. S. Miesch, M. Roth +3
We discuss recent observational, theoretical and modeling progress made in understanding the Sun's internal dynamics, including its rotation, meridional flow, convection and oversh…
Universality of the Small-Scale Dynamo Mechanism
R. Moll, J. Pietarila Graham, J. Pratt +3
We quantify possible differences between turbulent dynamo action in the Sun and the dynamo action studied in idealized simulations. For this purpose we compare Fourier-space shell-…
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…
Penumbral structure and outflows in simulated sunspots
M. Rempel, M. Schüssler, R. H. Cameron +1
Sunspots are concentrations of magnetic field on the visible solar surface that strongly affect the convective energy transport in their interior and surroundings. The filamentary…
Solar surface emerging flux regions: a comparative study of radiative MHD modeling and Hinode SOT observations
M. C. M. Cheung, M. Schuessler, T. D. Tarbell +1
We present results from numerical modeling of emerging flux regions on the solar surface. The modeling was carried out by means of 3D radiative MHD simulations of the rise of buoya…