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Modeling the Sun's open magnetic flux and the heliospheric current sheet
J. Jiang, R. Cameron, D. Schmitt +1
By coupling a solar surface flux transport model with an extrapolation of the heliospheric field, we simulate the evolution of the Sun's open magnetic flux and the heliospheric cur…
Properties of simulated sunspot umbral dots
L. Bharti, B. Beeck, M. Schuessler
Realistic 3D radiative MHD simulations reveal the magneto-convective processes underlying the formation of the photospheric fine structure of sunspots, including penumbral filament…
Simulation of a flux emergence event and comparison with observations by Hinode
L. Yelles Chaouche, M. C. M. Cheung, S. K. Solanki +2
We study the observational signature of flux emergence in the photosphere using synthetic data from a 3D MHD simulation of the emergence of a twisted flux tube. Several stages in t…
Comparison of the thin flux tube approximation with 3D MHD simulations
L. Yelles Chaouche, S. K. Solanki, M. Schuessler
The structure and dynamics of small vertical photospheric magnetic flux concentrations has been often treated in the framework of an approximation based upon a low-order truncation…
Magnetic field intensification: comparison of 3D MHD simulations with Hinode/SP results
S. Danilovic, M. Schüssler, S. K. Solanki
Recent spectro-polarimetric observations have provided detailed measurements of magnetic field, velocity and intensity during events of magnetic field intensification in the solar…
A comparison of measured and simulated solar network contrast
N. Afram, Y. C. Unruh, S. K. Solanki +2
Long-term trends in the solar spectral irradiance are important to determine the impact on Earth's climate. These long-term changes are thought to be caused mainly by changes in th…