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Study of the shower maximum depth by the method of detection of the EAS Cerenkov light pulse shape

Н. А. АлиевSamarkand Alisher Navoi State UnivT. A. AlimovM. K. KakhkharovN. K. KhakimovB. M. MakhmudovNailia R. RakhimovaR. T. TashpulatovG. B. KhristiansenMoscow State UniversityВ. В. ПросинMoscow State UniversityV. Yu. ZhukovMoscow State University

NASA Technical Reports Server (NASA)repository1985en

ABI

Annotatsiya

The results of processing the data on the shape of the EAS Cerenkov light pulses recorded by the extensive air showers (EAS) array are presented. The pulse FWHM is used to find the mean depth of EAS maximum.

Mavzular

Astrophysics and Cosmic Phenomena Radio Wave Propagation Studies Radio Astronomy Observations and Technology

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