Physics – Plasma Physics
Scientist
Physics
Plasma Physics
Scientist
Cross-Scale Science Study Team
Astronomical Institute and Institute of Atmospheric Physics, AS CR
Institute of Atmospheric Physics, Academy of Sciences Czech Republic, Prague, Czech Republic
Astronomical Institute, AS CR, Prague, Czech Republic
Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Institute of Atmospheric Physics, AS CR Prague, Czech Republic
Institute of Atmospheric Physics, Prague 4, Czech Republic
Astronomical Institute & Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, 14131 Prague, Czech Republic
Imperial College London, The Blackett Laboratory, London SW7 2AZ, UK
Institute of Atmospheric Physics, Academy of Sciences of Czech Republic, Prague, Czech Republic
Institute of Atmospheric Physics, AS CR, Bocni II / 1401, Prague 4, 141 31, Sporilov, Czech Republic
Department of Space Physics, Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Astronomy Institute, Academy of Sciences of Czech Republic, Prague, Czech Republic
Institute of Atmospheric Physics, ASCR, Prague, Czech Republic
Institute of Atmospheric Physics and Astronomical Institute, AS CR, Prague, Czech Republic
Astronomical Institute, ASCR, 14131 Prague, Czech Republic
Astronomical Institute, Academy of Sciences of the Czech Republic, Bocni II / 1401, 14131 Prague, Czech Republic; Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, Bocni II / 1401, 14131 Prague, Czech Republic
Astronomical Institute, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Dipartimento di Astronomia e Scienza dello Spazio, Università degli Studi di Firenze, Florence, Italy
Institute of Atmospheric Physics, Prague, Czech Republic, 14131
Institute of Atmospheric Physics, ASCR, Bocni II / 1401, Prague, 14131 Czech Republic of Atmospheric Physics, ASCR, Prague, 14131 Czech Repub
A Global Three Dimensional Hybrid Simulation of the Interaction Between a Magnetized Obstacle and the Solar Wind
A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind
Alfvén wave heating of heavy ions in the expanding solar wind: Hybrid simulations
Alfvénic Turbulence and Micro-Stream Structure in the Polar Solar Wind.
ARTEMIS Science Objectives
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