Long-term trends in cosmic rays and geomagnetic field secular variations

Autores
Elias, Ana Georgina; Zossi, Bruno Santiago; Gutierrez Falcon, Alvaro R.; Comedi, Emanuel S.; de Haro Barbás, Blas Federico
Año de publicación
2021
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Cosmic rays are modulated by solar and geomagnetic activity. In addition, the flux that arrives to theEarth is sensitive to the inner geomagnetic field through its effect on the geomagnetic cutoff rigidity, Rc. This field has been decaying globally at a rate of ~5% per century from at least 1840. However, due to its configuration and non-uniform trend around the globe, its secular variation during the last decades has induced negative and positive Rc trends depending on location. In the present work, the database from the World Data Center for Cosmic Rays (WDCCR) is used to analyze long-term trend variations linked to geomagnetic secular variations. This database includes more than 100 stations covering, some of them, almost seven decades since the 1950?s. Those stations spanning more than 20 years of data are selected for the present study in order to adequately filter solar activity effects.
Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Zossi, Bruno Santiago. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Gutierrez Falcon, Alvaro R.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Comedi, Emanuel S.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
XLVI Annual Seminar Physics of Auroral Phenomena
Apatity
Rusia
Russian Academy of Science. Polar Geophysical Institute
Materia
COSMIC RAYS
GEOMAGNETIC FIELD
SECULAR VARIATION
LONG TERM TRENDS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/225685
Acceder
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spelling Long-term trends in cosmic rays and geomagnetic field secular variationsElias, Ana GeorginaZossi, Bruno SantiagoGutierrez Falcon, Alvaro R.Comedi, Emanuel S.de Haro Barbás, Blas FedericoCOSMIC RAYSGEOMAGNETIC FIELDSECULAR VARIATIONLONG TERM TRENDShttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1Cosmic rays are modulated by solar and geomagnetic activity. In addition, the flux that arrives to theEarth is sensitive to the inner geomagnetic field through its effect on the geomagnetic cutoff rigidity, Rc. This field has been decaying globally at a rate of ~5% per century from at least 1840. However, due to its configuration and non-uniform trend around the globe, its secular variation during the last decades has induced negative and positive Rc trends depending on location. In the present work, the database from the World Data Center for Cosmic Rays (WDCCR) is used to analyze long-term trend variations linked to geomagnetic secular variations. This database includes more than 100 stations covering, some of them, almost seven decades since the 1950?s. Those stations spanning more than 20 years of data are selected for the present study in order to adequately filter solar activity effects.Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Zossi, Bruno Santiago. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Gutierrez Falcon, Alvaro R.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Comedi, Emanuel S.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaXLVI Annual Seminar Physics of Auroral PhenomenaApatityRusiaRussian Academy of Science. Polar Geophysical InstituteRussian Academy of Science. Polar Geophysical Institute2021info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSeminarioBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/225685Long-term trends in cosmic rays and geomagnetic field secular variations; XLVI Annual Seminar Physics of Auroral Phenomena; Apatity; Rusia; 2021; 79-80CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://pgia.ru:81/seminar/archive/2021/18_Elias.pdfinfo:eu-repo/semantics/altIdentifier/doi/10.51981/2588-0039.2021.44.018Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:37Zoai:ri.conicet.gov.ar:11336/225685instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:40:37.907CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Long-term trends in cosmic rays and geomagnetic field secular variations
title Long-term trends in cosmic rays and geomagnetic field secular variations
spellingShingle Long-term trends in cosmic rays and geomagnetic field secular variations
Elias, Ana Georgina
COSMIC RAYS
GEOMAGNETIC FIELD
SECULAR VARIATION
LONG TERM TRENDS
title_short Long-term trends in cosmic rays and geomagnetic field secular variations
title_full Long-term trends in cosmic rays and geomagnetic field secular variations
title_fullStr Long-term trends in cosmic rays and geomagnetic field secular variations
title_full_unstemmed Long-term trends in cosmic rays and geomagnetic field secular variations
title_sort Long-term trends in cosmic rays and geomagnetic field secular variations
dc.creator.none.fl_str_mv Elias, Ana Georgina
Zossi, Bruno Santiago
Gutierrez Falcon, Alvaro R.
Comedi, Emanuel S.
de Haro Barbás, Blas Federico
author Elias, Ana Georgina
author_facet Elias, Ana Georgina
Zossi, Bruno Santiago
Gutierrez Falcon, Alvaro R.
Comedi, Emanuel S.
de Haro Barbás, Blas Federico
author_role author
author2 Zossi, Bruno Santiago
Gutierrez Falcon, Alvaro R.
Comedi, Emanuel S.
de Haro Barbás, Blas Federico
author2_role author
author
author
author
dc.subject.none.fl_str_mv COSMIC RAYS
GEOMAGNETIC FIELD
SECULAR VARIATION
LONG TERM TRENDS
topic COSMIC RAYS
GEOMAGNETIC FIELD
SECULAR VARIATION
LONG TERM TRENDS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Cosmic rays are modulated by solar and geomagnetic activity. In addition, the flux that arrives to theEarth is sensitive to the inner geomagnetic field through its effect on the geomagnetic cutoff rigidity, Rc. This field has been decaying globally at a rate of ~5% per century from at least 1840. However, due to its configuration and non-uniform trend around the globe, its secular variation during the last decades has induced negative and positive Rc trends depending on location. In the present work, the database from the World Data Center for Cosmic Rays (WDCCR) is used to analyze long-term trend variations linked to geomagnetic secular variations. This database includes more than 100 stations covering, some of them, almost seven decades since the 1950?s. Those stations spanning more than 20 years of data are selected for the present study in order to adequately filter solar activity effects.
Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Zossi, Bruno Santiago. Universidad Nacional de Tucumán. Instituto de Física del Noroeste Argentino. - Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet Noa Sur. Instituto de Física del Noroeste Argentino; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Gutierrez Falcon, Alvaro R.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Comedi, Emanuel S.. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: de Haro Barbás, Blas Federico. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
XLVI Annual Seminar Physics of Auroral Phenomena
Apatity
Rusia
Russian Academy of Science. Polar Geophysical Institute
description Cosmic rays are modulated by solar and geomagnetic activity. In addition, the flux that arrives to theEarth is sensitive to the inner geomagnetic field through its effect on the geomagnetic cutoff rigidity, Rc. This field has been decaying globally at a rate of ~5% per century from at least 1840. However, due to its configuration and non-uniform trend around the globe, its secular variation during the last decades has induced negative and positive Rc trends depending on location. In the present work, the database from the World Data Center for Cosmic Rays (WDCCR) is used to analyze long-term trend variations linked to geomagnetic secular variations. This database includes more than 100 stations covering, some of them, almost seven decades since the 1950?s. Those stations spanning more than 20 years of data are selected for the present study in order to adequately filter solar activity effects.
publishDate 2021
dc.date.none.fl_str_mv 2021
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Seminario
Book
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/225685
Long-term trends in cosmic rays and geomagnetic field secular variations; XLVI Annual Seminar Physics of Auroral Phenomena; Apatity; Rusia; 2021; 79-80
CONICET Digital
CONICET
url http://hdl.handle.net/11336/225685
identifier_str_mv Long-term trends in cosmic rays and geomagnetic field secular variations; XLVI Annual Seminar Physics of Auroral Phenomena; Apatity; Rusia; 2021; 79-80
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://pgia.ru:81/seminar/archive/2021/18_Elias.pdf
info:eu-repo/semantics/altIdentifier/doi/10.51981/2588-0039.2021.44.018
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Russian Academy of Science. Polar Geophysical Institute
publisher.none.fl_str_mv Russian Academy of Science. Polar Geophysical Institute
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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