Monte Carlo Simulation and measurement of Calibration Neutron Monitor count rate dependence on proximity to water
dc.contributor.author | Duangjai B. | |
dc.contributor.author | Nuntiyakul W. | |
dc.contributor.author | Seripienlert A. | |
dc.contributor.author | Pagwhan A. | |
dc.contributor.author | Chaiwongkhot K. | |
dc.contributor.author | Sáiz A. | |
dc.contributor.author | Ruffolo D. | |
dc.contributor.author | Evenson P. | |
dc.contributor.correspondence | Duangjai B. | |
dc.contributor.other | Mahidol University | |
dc.date.accessioned | 2024-02-08T18:13:03Z | |
dc.date.available | 2024-02-08T18:13:03Z | |
dc.date.issued | 2023-01-01 | |
dc.description.abstract | Due to their global availability, neutron monitors play a crucial role in measuring time variations in the Galactic cosmic ray flux. A portable calibration neutron monitor (CalMon) is useful for intercalibrating various neutron monitors to ensure accurate measurements. A common technique to ensure that the calibration is done in a consistent environment is to place the CalMon at some height above a wide container (such as a portable swimming pool) filled with water. This study investigates the impact of CalMon height and water depth on the count rate ratio relative to a standard 18NM64 count rate recorded nearby (CalMon/18NM64). We compare simulated data from the FLUKA Monte Carlo package to experimental data from [1] to demonstrate the statistical accuracy of our simulation. Using the simulation results, we then extend the study of the proximity-to-water effect on the counting rate. In this work, we present a preliminary empirical model by analyzing the CalMon/18NM64 as a function of CalMon to water distance. Overall, our study enhances understanding of the response of calibration monitors (now often called “mini-neutron monitors”) operated in various locations worldwide, and validates the Monte Carlo techniques used to model the response of the global neutron monitor network. | |
dc.identifier.citation | Journal of Physics: Conference Series Vol.2653 No.1 (2023) | |
dc.identifier.doi | 10.1088/1742-6596/2653/1/012018 | |
dc.identifier.eissn | 17426596 | |
dc.identifier.issn | 17426588 | |
dc.identifier.scopus | 2-s2.0-85181986028 | |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/95755 | |
dc.rights.holder | SCOPUS | |
dc.subject | Physics and Astronomy | |
dc.title | Monte Carlo Simulation and measurement of Calibration Neutron Monitor count rate dependence on proximity to water | |
dc.type | Conference Paper | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85181986028&origin=inward | |
oaire.citation.issue | 1 | |
oaire.citation.title | Journal of Physics: Conference Series | |
oaire.citation.volume | 2653 | |
oairecerif.author.affiliation | National Astronomical Research Institute of Thailand | |
oairecerif.author.affiliation | University of Delaware | |
oairecerif.author.affiliation | Mahidol University | |
oairecerif.author.affiliation | Chiang Mai University |