Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astrophysical Inst. Potsdam, Potsdam, Germany
NRL
Astrophysical Institute Potsdam, Germany
Institute of Physics and Astronomy, University of Potsdam
NRL & University College London & Potsdam Univ
Astrophysika lisches Institut, D-14482 Potsdam, Germany
Zentralinstitut für Astrophysik, Potsdam, Germany
Space Science Division, Naval Research Laboratory, Washington, DC 20375-5352, USA; MSSL, University College London, Holmbury St. Mary, Dorking, Surrey, UK; Institut für Physik und Astronomie, Universität Potsdam, Potsdam, Germany
MSSL, UCL, United Kingdom
Mullard Space Science Laboratory, United Kingdom
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
University of Potsdam, Institute of Physics and Astronomy, Karl-Liebknecht-Str. 24 / 25, Potsdam, 14476, Germany; University College London, Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, United Kingdom für Astrophysik, Potsdam; Observatorium Weissenau, Tuebingen, Germany; IZMIRAN, Troitsk, Russia
Astrophysical Institute Potsdam
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany Institute Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Institute for Physics and Astronomy, University of Potsdam, Potsdam, Germany
Institut für Physik und Astronomie, University of Potsdam, Potsdam, Germany
Institute of Physics and Astronomy, University of Potsdam, Potsdam, Germany
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany; Kiepenheuer-Institut für Sonnenphysik, Schöneckstrasse 6, D-79104 Freiburg, Germany
Astrophysical Institute Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
School of Mathematics and Statistics, University of St. Andrews, St Andrews, Fife KY16 9SS, UK
Astrophysikalisches Insti
3D Reconstruction of a Rotating Erupting Prominence
3D Reconstruction of an Erupting Prominence
A Parametric Study of Erupting Flux Rope Rotation. Modeling the "Cartwheel CME" on 9 April 2008
A U-shaped, multiband, type II radio burst from a solar flare beyond the limb
Book-Review - Computational Plasma Physics - with Applications to Fusion and Astrophysics
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