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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/1874
Ver los metadatos del registro completo
id |
CONICETDig_fd389dcf2f43512055d5d256853a4484 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/1874 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
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 |
_version_ |
1844613063258406912 |
score |
13.070432 |