Modeling and Study of the Cerenkov Effect

The studies realized in INRNE (Institute for Nuclear Research and Nuclear Energy) particulary in cosmic rays detection and construction of Muonic Cerenkov Telescope in University of Blagoevgrad [1] shows the need to develop a theoretical model based on observed phenomenon and to refine it for the detection system optimisation. The effect was introduced in EGS4 code system. The first simulations were consecrated to different geometry of water tank in total reflection. The model was compared with experimental data realised with gamma source using the telescope. A simple atmospheric model is introduced in EGS4. The comparison between CORSIKA and EGS4 codes was realised.