Physics
Scientist
Charles University, Institute of Atmospheric Physics / CAS, Bocni II / 1401, CZ-14131 Praha 4, Prague, 14131 Czech Republic of Atmospheric Physics of the Academy of Sciences of the Czech Republic, Bocni II / 1401, 14131 Prague 4, Czech Republic.
Institute of Atmospheric Physics AS CR, Prague, Czech Republic
Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Institute of Atmospheric Physics, CAS, Prague, Czech Republic
Institute of Atmospheric Physics, Bocni II / 1401, CZ-14131 Praha 4, Prague, CZ-14131 Czech Republic of Atmospheric Physics, Academy of Sciences of the Czech Republic, Bocni II 1401, Prague, 141 31, Czech Republic
Institute of Atmospheric Physics, Bocni II / 1401, Praha 4, CZE 14131, Czech Republic
Institute of Atmospheric Physics, Bocni II / 1401, 14131 Praha 4, Czech Republic.
Institute of Atmospheric Physics, Bocni II, 14131 Prague, Czech Republic
Institute of Atmospheric Physics, Bocni II 1401, Prague, 141 31, Czech Republic
Institute of Atmospheric Physics, ASCR, Bocni II, 14131 Prague, Czech Republic
Institute of Atmospheric Physics, Prague, Czech Republic
Department of Aeronomy, Institute of Atmospheric Physics, Prague, Czech Republic
Institute of Atmospheric Physics, Bocni II / 1401, 14131 Prague, Czech Republic
Academy of Sciences of the Czech Republic, Institute of Atmospheric Physics, Prague, 199 99, Czech Republic of Atmospheric Phys., Prague, Czech Republic
Institute of Atmospheric Physics, ASCR, Prague, Czech Republic
Department of Upper Atmosphere, Institute of Atmospheric Physics, Prague, Czech Republic
Institute of Atmospheric Physics, Bocni II 1401, 141 31 Praha 4, Prague, Czech Republic
Analysis of subprotonospheric whistlers observed by DEMETER: A case study
Aoc of Magion Spacecraft as a Sub-Satellite in Interball Mission
Attitude Determination and Control of Motion around the Center of Mass of a Satellite and Subsatellite in the INTERBALL Project
Characteristic properties of Nu whistlers as inferred from observations and numerical modelling
Chorus source properties that produce time shifts and frequency range differences observed on different Cluster spacecraft
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