Publication Date:
2019-06-28
Description:
Fluctuations of the shower maximum depth obtained from analysis of electron and muon fluctuations and the extensive air showers (EAS) Cerenkov light on the Yakutsk array data and data of other arrays are considered. On the basis of these the estimation of composition of primaries with E sub 0 = 5.10 to the 17th power eV is received. Estimation of gamma-quanta flux with E sub 0 10 to the 17th power eV is given on the poor-muon showers.
Keywords:
SPACE RADIATION
Type:
OG-5.1-14
,
19th Intern. Cosmic Ray Conf - Vol. 2; p 186-189; NASA-CP-2376-VOL-2
Format:
application/pdf
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