Analysis of atmospheric pressure and temperature effects on cosmic ray measurements

Autores
De Mendonça, R. R. S.; Raulin, J. P.; Echer, E.; Makhmutov, V. S.; Fernandez, German Enzo Leonel
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this paper, we analyze atmospheric pressure and temperature effects on the records of the cosmic ray detector CARPET. This detector has monitored secondary cosmic ray intensity since 2006 at Complejo Astronómico El Leoncito (San Juan, Argentina, 31S, 69W, 2550m over sea level) where the geomagnetic rigidity cutoff, Rc, is ~9.8 GV. From the correlation between atmospheric pressure deviations and relative cosmic ray variations, we obtain a barometric coefficient of ?0.440.01 %/hPa. Once the data are corrected for atmospheric pressure, they are used to analyze temperature effects using four methods. Three methods are based on the surface temperature and the temperature at the altitude of maximum production of secondary cosmic rays. The fourth method, the integral method, takes into account the temperature height profile between 14 and 111 km above Complejo Astronómico El Leoncito. The results obtained from these four methods are compared on different time scales from seasonal time variations to scales related to the solar activity cycle. Our conclusion is that the integral method leads to better results to remove the temperature effect of the cosmic ray intensity observed at ground level.
Fil: De Mendonça, R. R. S.. National Institute for Space Research. Division of Space Geophysics; Brasil;
Fil: Raulin, J. P.. Universidade Presbiteriana Mackenzie; Brasil;
Fil: Echer, E.. National Institute for Space Research. Division of Space Geophysics; Brasil;
Fil: Makhmutov, V. S.. Russian Academy of Sciences. Lebedev Physical Institute; Rusia;
Fil: Fernandez, German Enzo Leonel. Consejo Nacional de Invest.cientif.y Tecnicas. Ctro Cientifico Tecnologico Conicet - San Juan. Complejo Astronomico;
Materia
COSMIC RAYS
PRESSURE EFFECT ON COSMIC RAYS
TEMPERATURE EFFECT ON COSMIC RAYS
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:11336/1874

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network_name_str CONICET Digital (CONICET)
spelling Analysis of atmospheric pressure and temperature effects on cosmic ray measurementsDe Mendonça, R. R. S.Raulin, J. P.Echer, E.Makhmutov, V. S.Fernandez, German Enzo LeonelCOSMIC RAYSPRESSURE EFFECT ON COSMIC RAYSTEMPERATURE EFFECT ON COSMIC RAYShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this paper, we analyze atmospheric pressure and temperature effects on the records of the cosmic ray detector CARPET. This detector has monitored secondary cosmic ray intensity since 2006 at Complejo Astronómico El Leoncito (San Juan, Argentina, 31S, 69W, 2550m over sea level) where the geomagnetic rigidity cutoff, Rc, is ~9.8 GV. From the correlation between atmospheric pressure deviations and relative cosmic ray variations, we obtain a barometric coefficient of ?0.440.01 %/hPa. Once the data are corrected for atmospheric pressure, they are used to analyze temperature effects using four methods. Three methods are based on the surface temperature and the temperature at the altitude of maximum production of secondary cosmic rays. The fourth method, the integral method, takes into account the temperature height profile between 14 and 111 km above Complejo Astronómico El Leoncito. The results obtained from these four methods are compared on different time scales from seasonal time variations to scales related to the solar activity cycle. Our conclusion is that the integral method leads to better results to remove the temperature effect of the cosmic ray intensity observed at ground level.Fil: De Mendonça, R. R. S.. National Institute for Space Research. Division of Space Geophysics; Brasil;Fil: Raulin, J. P.. Universidade Presbiteriana Mackenzie; Brasil;Fil: Echer, E.. National Institute for Space Research. Division of Space Geophysics; Brasil;Fil: Makhmutov, V. S.. Russian Academy of Sciences. Lebedev Physical Institute; Rusia;Fil: Fernandez, German Enzo Leonel. Consejo Nacional de Invest.cientif.y Tecnicas. Ctro Cientifico Tecnologico Conicet - San Juan. Complejo Astronomico;American Geophysical Union2013-04-30info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/1874De Mendonça, R. R. S.; Raulin, J. P.; Echer, E.; Makhmutov, V. S.; Fernandez, German Enzo Leonel; Analysis of atmospheric pressure and temperature effects on cosmic ray measurements; American Geophysical Union; Journal of Geophysical Research; 118; 4; 30-4-2013; 1403-14090148-0227enginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2012JA018026/fullinfo:eu-repo/semantics/altIdentifier/doi/10.1029/2012JA018026info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:34:22Zoai:ri.conicet.gov.ar:11336/1874instacron: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 09:34:22.734CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
title Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
spellingShingle Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
De Mendonça, R. R. S.
COSMIC RAYS
PRESSURE EFFECT ON COSMIC RAYS
TEMPERATURE EFFECT ON COSMIC RAYS
title_short Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
title_full Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
title_fullStr Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
title_full_unstemmed Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
title_sort Analysis of atmospheric pressure and temperature effects on cosmic ray measurements
dc.creator.none.fl_str_mv De Mendonça, R. R. S.
Raulin, J. P.
Echer, E.
Makhmutov, V. S.
Fernandez, German Enzo Leonel
author De Mendonça, R. R. S.
author_facet De Mendonça, R. R. S.
Raulin, J. P.
Echer, E.
Makhmutov, V. S.
Fernandez, German Enzo Leonel
author_role author
author2 Raulin, J. P.
Echer, E.
Makhmutov, V. S.
Fernandez, German Enzo Leonel
author2_role author
author
author
author
dc.subject.none.fl_str_mv COSMIC RAYS
PRESSURE EFFECT ON COSMIC RAYS
TEMPERATURE EFFECT ON COSMIC RAYS
topic COSMIC RAYS
PRESSURE EFFECT ON COSMIC RAYS
TEMPERATURE EFFECT ON COSMIC RAYS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this paper, we analyze atmospheric pressure and temperature effects on the records of the cosmic ray detector CARPET. This detector has monitored secondary cosmic ray intensity since 2006 at Complejo Astronómico El Leoncito (San Juan, Argentina, 31S, 69W, 2550m over sea level) where the geomagnetic rigidity cutoff, Rc, is ~9.8 GV. From the correlation between atmospheric pressure deviations and relative cosmic ray variations, we obtain a barometric coefficient of ?0.440.01 %/hPa. Once the data are corrected for atmospheric pressure, they are used to analyze temperature effects using four methods. Three methods are based on the surface temperature and the temperature at the altitude of maximum production of secondary cosmic rays. The fourth method, the integral method, takes into account the temperature height profile between 14 and 111 km above Complejo Astronómico El Leoncito. The results obtained from these four methods are compared on different time scales from seasonal time variations to scales related to the solar activity cycle. Our conclusion is that the integral method leads to better results to remove the temperature effect of the cosmic ray intensity observed at ground level.
Fil: De Mendonça, R. R. S.. National Institute for Space Research. Division of Space Geophysics; Brasil;
Fil: Raulin, J. P.. Universidade Presbiteriana Mackenzie; Brasil;
Fil: Echer, E.. National Institute for Space Research. Division of Space Geophysics; Brasil;
Fil: Makhmutov, V. S.. Russian Academy of Sciences. Lebedev Physical Institute; Rusia;
Fil: Fernandez, German Enzo Leonel. Consejo Nacional de Invest.cientif.y Tecnicas. Ctro Cientifico Tecnologico Conicet - San Juan. Complejo Astronomico;
description In this paper, we analyze atmospheric pressure and temperature effects on the records of the cosmic ray detector CARPET. This detector has monitored secondary cosmic ray intensity since 2006 at Complejo Astronómico El Leoncito (San Juan, Argentina, 31S, 69W, 2550m over sea level) where the geomagnetic rigidity cutoff, Rc, is ~9.8 GV. From the correlation between atmospheric pressure deviations and relative cosmic ray variations, we obtain a barometric coefficient of ?0.440.01 %/hPa. Once the data are corrected for atmospheric pressure, they are used to analyze temperature effects using four methods. Three methods are based on the surface temperature and the temperature at the altitude of maximum production of secondary cosmic rays. The fourth method, the integral method, takes into account the temperature height profile between 14 and 111 km above Complejo Astronómico El Leoncito. The results obtained from these four methods are compared on different time scales from seasonal time variations to scales related to the solar activity cycle. Our conclusion is that the integral method leads to better results to remove the temperature effect of the cosmic ray intensity observed at ground level.
publishDate 2013
dc.date.none.fl_str_mv 2013-04-30
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/11336/1874
De Mendonça, R. R. S.; Raulin, J. P.; Echer, E.; Makhmutov, V. S.; Fernandez, German Enzo Leonel; Analysis of atmospheric pressure and temperature effects on cosmic ray measurements; American Geophysical Union; Journal of Geophysical Research; 118; 4; 30-4-2013; 1403-1409
0148-0227
url http://hdl.handle.net/11336/1874
identifier_str_mv De Mendonça, R. R. S.; Raulin, J. P.; Echer, E.; Makhmutov, V. S.; Fernandez, German Enzo Leonel; Analysis of atmospheric pressure and temperature effects on cosmic ray measurements; American Geophysical Union; Journal of Geophysical Research; 118; 4; 30-4-2013; 1403-1409
0148-0227
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2012JA018026/full
info:eu-repo/semantics/altIdentifier/doi/10.1029/2012JA018026
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 American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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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