Physics – Plasma Physics
Scientist
Physics
Plasma Physics
Scientist
Swedish Institute of Space Physics, Uppsala, Sweden
Space Research Institute, Graz, Austria
Austrian Academy of Sciences, Space Research Institute, Schmiedlstrasse 6, 8042 Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Swedish Institute of Space Physics, Box 537, Uppsala, SE 751 21 Sweden Institute of Space Physics, Box 537, Uppsala, 75121 Sweden Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria
Swedish Institute of Space Physics, SE-751 21, Uppsala Sweden, Box 537 Sweden Institute of Space Physics, Box 537 SE-751 21 Uppsala, Sweden, Uppsala, SE-751 21 Sweden Institute of Space Physics, Box 537, Uppsala, SE-751 21 Sweden Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, Graz, 8042, Austria Research Institute Austrian Academy of Science, Schmiedlstr. 6, Graz, A-8042, Austria Research Institute, Austrian Academy of Sciences, Graz, 8042, Austria Academy of Sciences, Space Research Institute, Schmiedlstrasse 6, Graz, 8042, Austria Institute of Space Physics, Box 537, Uppsala, 751 21 Sweden Academy of Sciences, Space Research Institute, Graz, Austria Research Institute, Austrian Academy of Sciences, Graz, Austria Institute of Space Physics, Box 537, Uppsala, S-75121 Sweden
Swedish Institute of Space Physics, Box 537, Uppsala, SE 751 21 Sweden Institute of Space Physics, Box 537, Uppsala, SE- 75121 Sweden Academy of Sciences,
A case study of Kelvin-Helmholtz vortices on both flanks of the Earth's magnetotail
A New Method for Determining Whether Reconnection Occurs at a Current Sheet
Asymmetric plasma mixing via symmetrically developed vortices at the Earth's magnetopause
Cluster Multi-Scale Observation of MHD Shock-like Events in the Near-Earth Magnetotail
Cluster multispacecraft observations at the high-latitude duskside magnetopause: implications for continuous and component magnetic reconnection
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