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

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

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..195a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 195-198 (SEE N85-35968 24-93)

Computer Science

Cerenkov Radiation, Cosmic Ray Showers, Light (Visible Radiation), Pulse Amplitude, Pulsed Radiation, Data Processing, Digital Computers, Pulse Rate, Solar Arrays

Scientific paper

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.

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