Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina
- Autores
- Masías Meza, Jimmy Joel; Dasso, Sergio Ricardo
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The geomagnetic field (Bgeo) sets a lower cutoff rigidity (Rc) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton using different models for Bgeo (performed with the MAGCOS code), we use backtracking to analyze particles arriving at the location of two nodes of the net LAGO (Large Aperture Gamma ray burst Observatory) that will be built in the near future: Buenos Aires and Marambio (Antarctica), Argentina. We determine the asymptotic trajectories and the values of Rc for different incidence directions, for each node. Simulations were done using several models for Bgeo that emulate different geomagnetic conditions. The presented results will help to make analysis of future observations of the flux of cosmic rays done at these two LAGO nodes.
Fil: Masías Meza, Jimmy Joel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes 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 Ciencias Exactas y Naturales. Departamento de Física; Argentina - Materia
-
Cosmic Rays
Geomagnetism
Energetic Particles
Antarctica - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/16458
Ver los metadatos del registro completo
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Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, ArgentinaMasías Meza, Jimmy JoelDasso, Sergio RicardoCosmic RaysGeomagnetismEnergetic ParticlesAntarcticahttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The geomagnetic field (Bgeo) sets a lower cutoff rigidity (Rc) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton using different models for Bgeo (performed with the MAGCOS code), we use backtracking to analyze particles arriving at the location of two nodes of the net LAGO (Large Aperture Gamma ray burst Observatory) that will be built in the near future: Buenos Aires and Marambio (Antarctica), Argentina. We determine the asymptotic trajectories and the values of Rc for different incidence directions, for each node. Simulations were done using several models for Bgeo that emulate different geomagnetic conditions. The presented results will help to make analysis of future observations of the flux of cosmic rays done at these two LAGO nodes.Fil: Masías Meza, Jimmy Joel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes 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 Ciencias Exactas y Naturales. Departamento de Física; ArgentinaBBC SWS Regional Network2014-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16458Masías Meza, Jimmy Joel; Dasso, Sergio Ricardo; Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina; BBC SWS Regional Network; Sun and Geosphere; 9; 1; 1-2014; 41-471819-08392367-8852enginfo:eu-repo/semantics/reference/url/info:eu-repo/semantics/reference es info:eu-repo/semantics/reference/url/https://arxiv.org/abs/1402.6274info:eu-repo/semantics/altIdentifier/url/http://newserver.stil.bas.bg/SUNGEO//sun_geo_content.html#v91info:eu-repo/semantics/altIdentifier/url/http://newserver.stil.bas.bg/SUNGEO//00SGArhiv/SG_v9_No1_2014-pp-41-47.pdfinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1402.6274info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:49:18Zoai:ri.conicet.gov.ar:11336/16458instacron: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 09:49:18.944CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
title |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
spellingShingle |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina Masías Meza, Jimmy Joel Cosmic Rays Geomagnetism Energetic Particles Antarctica |
title_short |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
title_full |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
title_fullStr |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
title_full_unstemmed |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
title_sort |
Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina |
dc.creator.none.fl_str_mv |
Masías Meza, Jimmy Joel Dasso, Sergio Ricardo |
author |
Masías Meza, Jimmy Joel |
author_facet |
Masías Meza, Jimmy Joel Dasso, Sergio Ricardo |
author_role |
author |
author2 |
Dasso, Sergio Ricardo |
author2_role |
author |
dc.subject.none.fl_str_mv |
Cosmic Rays Geomagnetism Energetic Particles Antarctica |
topic |
Cosmic Rays Geomagnetism Energetic Particles Antarctica |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The geomagnetic field (Bgeo) sets a lower cutoff rigidity (Rc) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton using different models for Bgeo (performed with the MAGCOS code), we use backtracking to analyze particles arriving at the location of two nodes of the net LAGO (Large Aperture Gamma ray burst Observatory) that will be built in the near future: Buenos Aires and Marambio (Antarctica), Argentina. We determine the asymptotic trajectories and the values of Rc for different incidence directions, for each node. Simulations were done using several models for Bgeo that emulate different geomagnetic conditions. The presented results will help to make analysis of future observations of the flux of cosmic rays done at these two LAGO nodes. Fil: Masías Meza, Jimmy Joel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes 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 Ciencias Exactas y Naturales. Departamento de Física; Argentina |
description |
The geomagnetic field (Bgeo) sets a lower cutoff rigidity (Rc) to the entry of cosmic particles to Earth which depends on the geomagnetic activity. From numerical simulations of the trajectory of a proton using different models for Bgeo (performed with the MAGCOS code), we use backtracking to analyze particles arriving at the location of two nodes of the net LAGO (Large Aperture Gamma ray burst Observatory) that will be built in the near future: Buenos Aires and Marambio (Antarctica), Argentina. We determine the asymptotic trajectories and the values of Rc for different incidence directions, for each node. Simulations were done using several models for Bgeo that emulate different geomagnetic conditions. The presented results will help to make analysis of future observations of the flux of cosmic rays done at these two LAGO nodes. |
publishDate |
2014 |
dc.date.none.fl_str_mv |
2014-01 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/16458 Masías Meza, Jimmy Joel; Dasso, Sergio Ricardo; Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina; BBC SWS Regional Network; Sun and Geosphere; 9; 1; 1-2014; 41-47 1819-0839 2367-8852 |
url |
http://hdl.handle.net/11336/16458 |
identifier_str_mv |
Masías Meza, Jimmy Joel; Dasso, Sergio Ricardo; Geomagnetic effects on cosmic ray propagation under different conditions for Buenos Aires and Marambio, Argentina; BBC SWS Regional Network; Sun and Geosphere; 9; 1; 1-2014; 41-47 1819-0839 2367-8852 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/reference/url/info:eu-repo/semantics/reference es info:eu-repo/semantics/reference/url/https://arxiv.org/abs/1402.6274 info:eu-repo/semantics/altIdentifier/url/http://newserver.stil.bas.bg/SUNGEO//sun_geo_content.html#v91 info:eu-repo/semantics/altIdentifier/url/http://newserver.stil.bas.bg/SUNGEO//00SGArhiv/SG_v9_No1_2014-pp-41-47.pdf info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1402.6274 |
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.publisher.none.fl_str_mv |
BBC SWS Regional Network |
publisher.none.fl_str_mv |
BBC SWS Regional Network |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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