Abstract
The problem of PCR Composition at super high energies is far from being solved.EAS Cherenkov light spatial-angular distribution (CL SAD) can yield important information on the primary mass. In order to use EAS CL SAD for the study of PCR composition one needs a set of imaging telescopes with the appropriate parameters supported by a dense net of fast optical detectors capable of measuring EAS Cherenkov light pulses. On the basis of full Monte-Carlo simulations the pixel size of imaging telescopes is optimized for a specific observation level ∼4km which is typical for the Eastern Pamir mountains.
Highlights
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Summary
× Ñ Ð Öo ÁÒØ Ö Ø ÓÒ × ÑÔÓÖØ ÒØ ÓÖ Ô ÖØ Ð ×ÙÔÔÖ ×× Ó Ù ØÙ Ø ÓÒ× ÙØ Ø Ô× ÑÙ×Ø ÒÓØ ØÓÓ Û o ÁÒ Ø × Ô ÖØ ÙÐ Ö × Ô × 5o ÐÓÒ 1o Û o ÁÑ1. ØÙÖ × Û Ö ÓÖÑ × Ô ÖØ Ð ÒØ Ö Ð Si Ö Ø Ó× rij = Si/Sj, i = jo r13 Ò r24 Û Ö Ù× Ò Ø × Ð1 ÙÐ Ø ÓÒ Û Ó × ÒÓØ Ñ Ò Ø × Ö Ø ÓÔØ ÑÙÑ.
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