Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity

Neutron monitors are a standard tool for high-precision monitoring of changes in the Galactic cosmic ray (GCR) flux that occur as a result of variations of the heliospheric conditions and solar storms. In Thailand, we have developed a mobile neutron monitor named “Changvan” based on the 3NM64 design...

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Main Authors: S. Khamphakdee, W. Nuntiyakul, C. Banglieng, A. Seripienlert, P. Yakum, A. Sáiz, D. Ruffolo, P. Evenson, K. Munakata, S. Komonjinda
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adc5f9
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author S. Khamphakdee
W. Nuntiyakul
C. Banglieng
A. Seripienlert
P. Yakum
A. Sáiz
D. Ruffolo
P. Evenson
K. Munakata
S. Komonjinda
author_facet S. Khamphakdee
W. Nuntiyakul
C. Banglieng
A. Seripienlert
P. Yakum
A. Sáiz
D. Ruffolo
P. Evenson
K. Munakata
S. Komonjinda
author_sort S. Khamphakdee
collection DOAJ
description Neutron monitors are a standard tool for high-precision monitoring of changes in the Galactic cosmic ray (GCR) flux that occur as a result of variations of the heliospheric conditions and solar storms. In Thailand, we have developed a mobile neutron monitor named “Changvan” based on the 3NM64 design, except that the middle counter lacks lead producer rings, so we call it a semileaded neutron monitor. From 2021 April to 2023 April, the Changvan operated at the Science and Technology Park, Mae Hia, Chiang Mai, Thailand, at an altitude of about 340 m above sea level, with a vertical cutoff rigidity of 16.7 GV, which is near the highest value observed globally. With a similar cutoff rigidity, the nearby Princess Sirindhorn Neutron Monitor is an 18NM64 at the summit of Doi Inthanon, the highest mountain in Thailand, at 2560 m above sea level. We examine how count rates at different altitudes with similar cutoffs, count rates from the unleaded versus leaded counters, and the leader fraction measured from time-delay histograms all reflect GCR spectral differences, thus providing a variety of techniques for tracking cosmic-ray spectral changes. Applied at high cutoff rigidity, these methods extend the reach of the worldwide neutron monitor network to even higher rigidity.
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spelling doaj-art-c1fd680146cf447ab5bed1ceb019e3a32025-08-20T02:28:19ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198415110.3847/1538-4357/adc5f9Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff RigidityS. Khamphakdee0https://orcid.org/0009-0008-8182-1180W. Nuntiyakul1https://orcid.org/0000-0002-1664-5845C. Banglieng2https://orcid.org/0000-0002-4862-2015A. Seripienlert3https://orcid.org/0000-0002-3764-8949P. Yakum4https://orcid.org/0009-0000-7520-3038A. Sáiz5https://orcid.org/0000-0001-7771-4341D. Ruffolo6https://orcid.org/0000-0003-3414-9666P. Evenson7https://orcid.org/0000-0001-7929-810XK. Munakata8https://orcid.org/0000-0002-2131-4100S. Komonjinda9https://orcid.org/0000-0001-7987-017XGraduate Program in Astronomy, Department of Physics and Materials Science, Faculty of Science, Chiang Mai University , Chiang Mai 50200, ThailandDepartment of Physics and Materials Science, Faculty of Science, Chiang Mai University , Chiang Mai 50200, Thailand ; waraporn.n@cmu.ac.thDivision of Physics, Faculty of Science and Technology, Rajamangala University of Technology Thanyaburi , Pathum Thani 12110, ThailandOffice of Research Administration, Chiang Mai University , Chiang Mai 50200, ThailandGraduate Program in Astronomy, Department of Physics and Materials Science, Faculty of Science, Chiang Mai University , Chiang Mai 50200, ThailandDepartment of Physics, Faculty of Science, Mahidol University , Bangkok 10400, ThailandDepartment of Physics, Faculty of Science, Mahidol University , Bangkok 10400, ThailandDepartment of Physics and Astronomy, University of Delaware , Newark, DE 19716, USAPhysics Department, Shinshu University , Matsumoto, Nagano 390-8621, JapanDepartment of Physics and Materials Science, Faculty of Science, Chiang Mai University , Chiang Mai 50200, Thailand ; waraporn.n@cmu.ac.thNeutron monitors are a standard tool for high-precision monitoring of changes in the Galactic cosmic ray (GCR) flux that occur as a result of variations of the heliospheric conditions and solar storms. In Thailand, we have developed a mobile neutron monitor named “Changvan” based on the 3NM64 design, except that the middle counter lacks lead producer rings, so we call it a semileaded neutron monitor. From 2021 April to 2023 April, the Changvan operated at the Science and Technology Park, Mae Hia, Chiang Mai, Thailand, at an altitude of about 340 m above sea level, with a vertical cutoff rigidity of 16.7 GV, which is near the highest value observed globally. With a similar cutoff rigidity, the nearby Princess Sirindhorn Neutron Monitor is an 18NM64 at the summit of Doi Inthanon, the highest mountain in Thailand, at 2560 m above sea level. We examine how count rates at different altitudes with similar cutoffs, count rates from the unleaded versus leaded counters, and the leader fraction measured from time-delay histograms all reflect GCR spectral differences, thus providing a variety of techniques for tracking cosmic-ray spectral changes. Applied at high cutoff rigidity, these methods extend the reach of the worldwide neutron monitor network to even higher rigidity.https://doi.org/10.3847/1538-4357/adc5f9Cosmic ray detectorsGalactic cosmic raysSpace weatherSolar-terrestrial interactions
spellingShingle S. Khamphakdee
W. Nuntiyakul
C. Banglieng
A. Seripienlert
P. Yakum
A. Sáiz
D. Ruffolo
P. Evenson
K. Munakata
S. Komonjinda
Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
The Astrophysical Journal
Cosmic ray detectors
Galactic cosmic rays
Space weather
Solar-terrestrial interactions
title Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
title_full Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
title_fullStr Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
title_full_unstemmed Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
title_short Methods for Tracking Cosmic-Ray Spectral Changes Using Neutron Monitors at High Cutoff Rigidity
title_sort methods for tracking cosmic ray spectral changes using neutron monitors at high cutoff rigidity
topic Cosmic ray detectors
Galactic cosmic rays
Space weather
Solar-terrestrial interactions
url https://doi.org/10.3847/1538-4357/adc5f9
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