A Selection of Different Cosmic Ray Primaries Using a New Selection Parameter Based on Cerenkov Light Registration

Physics

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Scientific paper

In the field of cosmic ray investigations are few very important problems to resolve. One of them is the precise determination of the primary cosmic ray energy spectra in the very interesting region of the knee. One possible method is based on Cerenkov light from extensive air showers measurements. It is very important to propose methods and techniques, which gives the possibility to obtain huge statistics or not used previously. One of the most important problems in experimental studies is the selection with constant efficiency of extensive air showers. In this work using previously proposed selection parameter based only on Cerenkov light registration different detector configurations are investigated. To use this parameter is very important to determine with big precision the shower axis at given observation level. The influence of the shower axis determination accuracies is investigated.

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