Abstract
Data on the EAS neutron component obtained using the PRISMA-32 array are presented. Secondary neutrons are first moderated and then detected by specialized scintillation electron–neutron detectors (en-detectors) within 20 ms of the arrival of the shower front. The PRISMA-32 array comprises 32 en-detectors and has been operated in the continuous data acquisition mode for more than five years.
Similar content being viewed by others
REFERENCES
Yu. V. Stenkin and J. F. Valdes-Galicia, in Proc. 27th Int. Cosmic Ray Conf., Hamburg, Germany, 2001, Vol. 4, p. 1453.
D. M. Gromushkin et al., J. Instrum. 9, C08028 (2014).
A. A. Petrukhin, Phys.-Usp. 58, 486 (2015).
Yu. V. Stenkin et al., Chin. Phys. C 37, 015001 (2013).
J. R. Hörandel et al., in Proc. 27th Int. Cosmic Ray Conf., Hamburg, Germany, 2001, Vol. 1, p. 137.
ACKNOWLEDGMENTS
This study was conducted at the unique scientific facility “Experimental Complex NEVOD” and supported by grant MK-7597.2016.2 from the President of the Russian Federation for state support of young Russian candidates of sciences.
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated by D. Safin
Rights and permissions
About this article
Cite this article
Gromushkin, D.M., Bogdanov, F.A., Stenkin, Y.V. et al. Investigation of the EAS Neutron Component with the PRISMA-32 Array. Phys. Part. Nuclei 49, 602–606 (2018). https://doi.org/10.1134/S1063779618040275
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063779618040275