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arxiv: 1612.09460 · v1 · pith:DIUJMT5Knew · submitted 2016-12-30 · 🌌 astro-ph.IM · astro-ph.HE

Characteristics of EAS neutron component obtained with PRISMA-32 array

classification 🌌 astro-ph.IM astro-ph.HE
keywords arrayneutronneutronsresultscomponentdistributionprisma-32showers
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The paper is devoted to the results of the EAS neutron component investigations by means of the PRISMA-32 array. The array consists of 32 en-detectors and enables to record delayed thermal neutrons accompanying showers. For registration of thermal neutrons, the scintillator based on $^{6}Li$ isotope as a target is used in the detectors. Some results of the processing of data accumulated over a long period of time are presented: the lateral distribution function of neutrons in EAS and preliminary results on EAS neutron multiplicity spectrum and distribution of showers in e/n ratio.

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