Multiple Particle Detection in a Neutron Monitor

Magnetic activity on the sun influences the flux of galactic cosmic rays at Earth in the process known as solar modulation. While most pronounced at 1 GeV and below, it also operates at much higher energy, still exhibiting solar magnetic polarity dependence. Historically, an observational gap exists...

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主要作者: Evenson P.
其他作者: Mahidol University
格式: Conference or Workshop Item
出版: 2023
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spelling th-mahidol.865792023-06-19T01:06:36Z Multiple Particle Detection in a Neutron Monitor Evenson P. Mahidol University Multidisciplinary Magnetic activity on the sun influences the flux of galactic cosmic rays at Earth in the process known as solar modulation. While most pronounced at 1 GeV and below, it also operates at much higher energy, still exhibiting solar magnetic polarity dependence. Historically, an observational gap exists between approximately 17 GeV (the highest geomagnetic cutoff) neutron monitor data and muon observations of primary cosmic rays that are mostly above 50 GeV. Detecting multiple neutrons from the same primary particle has recently been used to monitor the primary energy spectrum using data from a single neutron monitor. Over the past few years we have used details of the timing distribution from individual neutron detectors and pairwise correlations among adjacent detectors to improve the energy resolution of this technique. We present a further extension of our observations to pattern recognition of events comprising hits in multiple detectors in order to identify and study cases where more than one secondary particle from the same primary interacts in the neutron monitor. Our particular focus at present is to distinguish interactions of energetic hadrons from those generated by cores of small air showers. 2023-06-18T18:06:36Z 2023-06-18T18:06:36Z 2022-03-18 Conference Paper Proceedings of Science Vol.395 (2022) 18248039 2-s2.0-85144108416 https://repository.li.mahidol.ac.th/handle/123456789/86579 SCOPUS
institution Mahidol University
building Mahidol University Library
continent Asia
country Thailand
Thailand
content_provider Mahidol University Library
collection Mahidol University Institutional Repository
topic Multidisciplinary
spellingShingle Multidisciplinary
Evenson P.
Multiple Particle Detection in a Neutron Monitor
description Magnetic activity on the sun influences the flux of galactic cosmic rays at Earth in the process known as solar modulation. While most pronounced at 1 GeV and below, it also operates at much higher energy, still exhibiting solar magnetic polarity dependence. Historically, an observational gap exists between approximately 17 GeV (the highest geomagnetic cutoff) neutron monitor data and muon observations of primary cosmic rays that are mostly above 50 GeV. Detecting multiple neutrons from the same primary particle has recently been used to monitor the primary energy spectrum using data from a single neutron monitor. Over the past few years we have used details of the timing distribution from individual neutron detectors and pairwise correlations among adjacent detectors to improve the energy resolution of this technique. We present a further extension of our observations to pattern recognition of events comprising hits in multiple detectors in order to identify and study cases where more than one secondary particle from the same primary interacts in the neutron monitor. Our particular focus at present is to distinguish interactions of energetic hadrons from those generated by cores of small air showers.
author2 Mahidol University
author_facet Mahidol University
Evenson P.
format Conference or Workshop Item
author Evenson P.
author_sort Evenson P.
title Multiple Particle Detection in a Neutron Monitor
title_short Multiple Particle Detection in a Neutron Monitor
title_full Multiple Particle Detection in a Neutron Monitor
title_fullStr Multiple Particle Detection in a Neutron Monitor
title_full_unstemmed Multiple Particle Detection in a Neutron Monitor
title_sort multiple particle detection in a neutron monitor
publishDate 2023
url https://repository.li.mahidol.ac.th/handle/123456789/86579
_version_ 1781414485696708608