Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany;
MPI fuer Sonnensystemforschung, Katlenburg-Lindau, Germany;
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany
Max-Planck-Institut für Sonnensystemforschung, Germany
MPS, Max-Planck Str. 2, Katlenburg-Lindau, 37191, Germany
MPS, Max-Planck-Str. 2, Katlenburg-Lindau, 37191, Germany
Max Planck Institute for Solar System Research, Germany
Max Planck Institutur Sonnensystemforschung, Germany
MPI, Germany
MPS, Max-Planck-Str. 2, lenburg-Lindau, 37191, Germany
MPS, Max-Planck-St. 2, Katlenburg-Lindau, 37191, Germany
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, Katlenburg-Lindau, 37191, Germany für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany
Max Planck Institute for Solar System Research, Max-Planck-Str.2, Katlenburg-Lindau, LS 37191, Germany
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, Katlenburg-Lindau, 37191, Germany
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, Katlenburg- Lindau, NI 37191, Germany
Max-Planck-Institute for Solar System Research, Max-Planck Str. 2, Katlenburg-Lindau, 37191, Germany
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
Max-Planck-Institut für Sonnensystemforschung
Max-Planck-Institute for Solar System Research, Katlenburg-Lindau, Germany
School of Mathematics and Statistics, University of St. Andrews, St. Andrews, KY16 9SS, UK
Max-Planck-Institute for Solar System Research, Germany
MPS, Germany
3D Magnetic Field Configuration of the 2006 December 13 Flare Extrapolated with the Optimization Method
3D Reconstruction of Polar Plumes From STEREO/SECCHI Images.
A comparison of preprocessing methods for solar force-free magnetic field extrapolation
A filament supported by different magnetic field configurations
A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum
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