Publication Date:
2019-06-28
Description:
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.
Keywords:
SPACE RADIATION
Type:
HE-4.4-15
,
19th Intern. Cosmic Ray Conf - Vol. 7; p 195-198; NASA-CP-2376-VOL-7
Format:
application/pdf
Permalink