Computer Science
Scientist
Institute of Atmospheric Physics ASCR, Upper Atmosphere, Prague, Czech Republic
Institute of Atmospheric Physics, Bocni II, 141 31 Praha 4, Czech Republic
Lags in in the correlation between the solar activity and upper ionosphere characteristics.
Time delays in the correlation between solar activity and the F2 region plasma frequency
Variations of daytime and nighttime electron temperature and heat flux in the upper ionosphere, topside ionosphere and lower plasmasphere for low and high solar activity
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