First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base

A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs duri...

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Published in:Advances in Space Research
Main Authors: Santos, Noelia Ayelen, Dasso, Sergio Ricardo, Gulisano, Adriana Maria, Areso, Omar Antonio, Pereira, Matias Hernan, Asorey, Hernán Gonzalo, Rubinstein, Lucas
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier
Subjects:
Online Access:http://hdl.handle.net/11336/218041
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author Santos, Noelia Ayelen
Dasso, Sergio Ricardo
Gulisano, Adriana Maria
Areso, Omar Antonio
Pereira, Matias Hernan
Asorey, Hernán Gonzalo
Rubinstein, Lucas
author_facet Santos, Noelia Ayelen
Dasso, Sergio Ricardo
Gulisano, Adriana Maria
Areso, Omar Antonio
Pereira, Matias Hernan
Asorey, Hernán Gonzalo
Rubinstein, Lucas
author_sort Santos, Noelia Ayelen
collection CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas)
container_issue 6
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container_title Advances in Space Research
container_volume 71
description A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth's rotation combined with the spatial anisotropy of the GCR flux; and (b) ∼ 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is ∼ 0.08% and the maximum flux is observed in ∼ 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth. Fil: Santos, Noelia Ayelen. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Ciencias de la Atmósfera y los Océanos; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina Fil: Dasso, Sergio Ricardo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de ...
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geographic Antarctic
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spelling ftconicet:oai:ri.conicet.gov.ar:11336/218041 2025-01-16T19:42:22+00:00 First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base Santos, Noelia Ayelen Dasso, Sergio Ricardo Gulisano, Adriana Maria Areso, Omar Antonio Pereira, Matias Hernan Asorey, Hernán Gonzalo Rubinstein, Lucas application/pdf http://hdl.handle.net/11336/218041 eng eng Elsevier info:eu-repo/semantics/altIdentifier/url/https://linkinghub.elsevier.com/retrieve/pii/S0273117722010730 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.asr.2022.11.041 http://hdl.handle.net/11336/218041 CONICET Digital CONICET info:eu-repo/semantics/restrictedAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ COSMIC RAY DETECTOR COSMIC RAY SOLAR MODULATION SPACE WEATHER https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion ftconicet https://doi.org/10.1016/j.asr.2022.11.041 2024-10-04T09:34:17Z A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth's rotation combined with the spatial anisotropy of the GCR flux; and (b) ∼ 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is ∼ 0.08% and the maximum flux is observed in ∼ 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth. Fil: Santos, Noelia Ayelen. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Ciencias de la Atmósfera y los Océanos; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina Fil: Dasso, Sergio Ricardo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universidad de Buenos Aires. Facultad de ... Article in Journal/Newspaper Antarc* Antarctic CONICET Digital (Consejo Nacional de Investigaciones Científicas y Técnicas) Antarctic Argentina Argentine Marambio ENVELOPE(-56.750,-56.750,-64.283,-64.283) Ricardo ENVELOPE(-63.033,-63.033,-64.867,-64.867) Advances in Space Research 71 6 2967 2976
spellingShingle COSMIC RAY DETECTOR
COSMIC RAY SOLAR MODULATION
SPACE WEATHER
https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
Santos, Noelia Ayelen
Dasso, Sergio Ricardo
Gulisano, Adriana Maria
Areso, Omar Antonio
Pereira, Matias Hernan
Asorey, Hernán Gonzalo
Rubinstein, Lucas
First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title_full First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title_fullStr First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title_full_unstemmed First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title_short First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base
title_sort first measurements of periodicities and anisotropies of cosmic ray flux observed with a water-cherenkov detector at the marambio antarctic base
topic COSMIC RAY DETECTOR
COSMIC RAY SOLAR MODULATION
SPACE WEATHER
https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
topic_facet COSMIC RAY DETECTOR
COSMIC RAY SOLAR MODULATION
SPACE WEATHER
https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
url http://hdl.handle.net/11336/218041