Physics – Space Physics
Scientist
Physics
Space Physics
Scientist
Department of Physics and Astronomy, The University of Iowa, Iowa City, IA, USA; Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic
University of Iowa, Department of Physics and Astronomy, Iowa City, IA 52242, USA; Charles University, Faculty of Mathematics and Physics, Prague, CZ-18000 Czech Republic
The University of Iowa, Department of Physics and Astronomy, Iowa City, IA 52242, USA; Charles University, Faculty of Mathematics and Physics, Prague, 18000 Czech Republic
Charles University and IAP, ASCR, Prague, 18000 Czech Republic
Charles University, Institute of Atmospheric Physics / CAS, Bocni II / 1401, CZ-14131 Praha 4, Prague, 14131 Czech Republic University, Faculty of Mathematics and Physics, Prague, Czech Republic
Institute of Atmospheric Physics AS CR, Prague, Czech Republic
IAP, ASCR, Prague, Czech Republic;
Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa, USA
Charles Univ., Prague, Czech Republic
Department of Space Physics, Institute of Atmospheric Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Institute of Atmospheric Physics, Czech Academay of Sciences, Prague, Czech Republic
Charles University, V Holesovickach 2, CZ-18000 Praha 8, Prague, CZ-18000 Czech Republic
Charles University, Faculty of Mathematics and Physics, Prague, 18000 Czech Republic; IAP, CAS, Prague, 141 31 Czech Republic
Charles University, Fac Mathematics & Physics V Holesovickach 2, Prague 8, CZ-18000 Czech Republic University, Faculty of Mathematics and Physics, V Holesovickach 2, Prague, CZ-18000 Czech Republic
Faculty of Mathematics and Physics, Charles University, Prague and IAP / ASCR, Prague, Czech Republic
Institute of Atmospheric Physics, ASCR, Prague, Czech Republic
Charles University, Faculty of Mathematics and Physics, P
A comparison of the rotational modulation of three types of Saturnian radio emissions
A Diffusive Equilibrium Density Model for a Two-Species Plasma in Saturn's Magnetosphere
A diffusive equilibrium model for the plasma density in Saturn's magnetosphere
A microscopic and nanoscopic view of storm-time chorus
A microscopic and nanoscopic view of storm-time chorus on 31 March 2001
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Profile ID: LFWR-SCP-P-346002