Physics
Scientist
Institut für Geophysik und Meteorologie, Universität Köln, Albertus-Magnus-Platz, Köln, 50923 Germany
Institut für Geophysik and Meterologie, Universität zu Köln, Köln
Institut für Geophysik und Meteorologie, Universität zu Köln, Cologne, Germany
Institut für Geophysik und Meteorologie, Universität zu Köln, Albertus-Magnus-Platz, 50923 Köln, Germany Universität, Germany
Bonn Univ., Germany
Cologne University
Institute of Geophysics and Meteorology, University of Cologne, Germany of Geophysics and Meteorology, University of Cologne, Institute of Geophysics and Meteorology, University of Cologne, Cologne, D-50923, Germany
U. Köln
Institute of Geophysics and Meteorology, University of Cologne, Germany, D-50923
Institute of Geophysics and Meteorology, University of Cologne, Albertus Magnus Platz, Köln, 50923 Germany of Geophysics & Meteorology, University of Cologne, Köln, Germany
Institute of Geophysics and Meteorology, University of Köln, Albertus-Magnus-Platz, Köln, 50923, Germany
Radioastronomisches Institut der Universität Bonn, Auf dem Huegel 71, D-53121 Bonn, Germany; Institut für Geophysik und Meteorologie, Universität zu Köln, Albertus-Magnus-Platz, D-50923 Köln, Germany
Institut für Geophysik und Meterologie, Universität zu Köln, Albertus-Magnus-Platz, Köln D-50923, Germany
Institute of Geophysics and Meteorology, Universität zu Köln, Köln, Germany
University of Cologne, Köln, Germany
Institute of Geophysics and Meteorology, University of Cologne, Koeln, Germany;
Institute for Geophysics, University of Cologne, Colgne, Germany;
Sterrewacht Leiden, Leiden, Netherlands
A Search for Dust Devils on Mars
A very dense H I filament within the Local Hot Bubble
Cassini Magnetic Field Observations During the Close Titan Encounter on October 26, 2004 on October 26, 2004
Der Leonidenschauer. Ein Risiko für die Raumfahrt?
Derivation of the forward velocity of martian dust devils and their comparison with Wind profiles from of a general circulation model
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