A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)

Autores
Azpilicueta, Francisco Javier; Altadill, D.; Brunini, Claudio Antonio; Torta, J. M.; Blanch, Eva Valeria
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
During the last decade the amount of ionosphere measurements, from ground and space born sources, has substantially increased along with the development of high end processing systems. This constitutes a perfect scenario for the International Reference Ionosphere (IRI) to assimilate this huge new database and to satisfy the new needs of the aeronomic community: an IRI with meteorological capability. The first step before the implementation of an assimilative procedure is to validate the new data. This work intends to contribute in this direction by studying the differences (systematic and statistical) between the F2 peak parameters (hmF2 and NmF2) predicted by the IRI(CCIR) and those obtained from the electron density profiles computed with LPIM-COSMIC/Formosat3 (LPIM-C/F3) technique. The analyzed period extends from January 2007 to October 2012, thus covering all the different seasonal Sun–Earth configurations and a range of solar activity going from low to mid-high level. The analysis shows that there is no significant systematic bias between the IRI and LPIM-C/F3 values on both parameters. The obtained differences are comparable to those found between IRI and other models and data sources. In addition a correlation with the solar activity level is observed. The analysis performed is also helpful to study and asses the potentiality of the meteorological information contained in the LPIM-C/F3 by analyzing the standard deviation of the differences. This extra information could represent the key element to improve the IRI predicting capabilities.
Fil: Azpilicueta, Francisco Javier. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Altadill, D.. Universitat Ramon Llull; España
Fil: Brunini, Claudio Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Torta, J. M.. Universitat Ramon Llull; España
Fil: Blanch, Eva Valeria. Universitat Ramon Llull; España
Materia
Ionosphere
Iri
Lpim
Cosmic/F3 Mission
Nmf2 And Hmf2
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:11336/32565
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)Azpilicueta, Francisco JavierAltadill, D.Brunini, Claudio AntonioTorta, J. M.Blanch, Eva ValeriaIonosphereIriLpimCosmic/F3 MissionNmf2 And Hmf2https://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1During the last decade the amount of ionosphere measurements, from ground and space born sources, has substantially increased along with the development of high end processing systems. This constitutes a perfect scenario for the International Reference Ionosphere (IRI) to assimilate this huge new database and to satisfy the new needs of the aeronomic community: an IRI with meteorological capability. The first step before the implementation of an assimilative procedure is to validate the new data. This work intends to contribute in this direction by studying the differences (systematic and statistical) between the F2 peak parameters (hmF2 and NmF2) predicted by the IRI(CCIR) and those obtained from the electron density profiles computed with LPIM-COSMIC/Formosat3 (LPIM-C/F3) technique. The analyzed period extends from January 2007 to October 2012, thus covering all the different seasonal Sun–Earth configurations and a range of solar activity going from low to mid-high level. The analysis shows that there is no significant systematic bias between the IRI and LPIM-C/F3 values on both parameters. The obtained differences are comparable to those found between IRI and other models and data sources. In addition a correlation with the solar activity level is observed. The analysis performed is also helpful to study and asses the potentiality of the meteorological information contained in the LPIM-C/F3 by analyzing the standard deviation of the differences. This extra information could represent the key element to improve the IRI predicting capabilities.Fil: Azpilicueta, Francisco Javier. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Altadill, D.. Universitat Ramon Llull; EspañaFil: Brunini, Claudio Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Torta, J. M.. Universitat Ramon Llull; EspañaFil: Blanch, Eva Valeria. Universitat Ramon Llull; EspañaElsevier2014-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/32565Torta, J. M.; Blanch, Eva Valeria; Azpilicueta, Francisco Javier; Altadill, D.; Brunini, Claudio Antonio; A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR); Elsevier; Advances in Space Research; 55; 8; 7-2014; 2012-20190273-1177CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.asr.2014.08.008info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0273117714005201info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:32:56Zoai:ri.conicet.gov.ar:11336/32565instacron: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:34982025-10-15 15:32:56.298CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
title A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
spellingShingle A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
Azpilicueta, Francisco Javier
Ionosphere
Iri
Lpim
Cosmic/F3 Mission
Nmf2 And Hmf2
title_short A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
title_full A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
title_fullStr A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
title_full_unstemmed A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
title_sort A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR)
dc.creator.none.fl_str_mv Azpilicueta, Francisco Javier
Altadill, D.
Brunini, Claudio Antonio
Torta, J. M.
Blanch, Eva Valeria
author Azpilicueta, Francisco Javier
author_facet Azpilicueta, Francisco Javier
Altadill, D.
Brunini, Claudio Antonio
Torta, J. M.
Blanch, Eva Valeria
author_role author
author2 Altadill, D.
Brunini, Claudio Antonio
Torta, J. M.
Blanch, Eva Valeria
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ionosphere
Iri
Lpim
Cosmic/F3 Mission
Nmf2 And Hmf2
topic Ionosphere
Iri
Lpim
Cosmic/F3 Mission
Nmf2 And Hmf2
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.5
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv During the last decade the amount of ionosphere measurements, from ground and space born sources, has substantially increased along with the development of high end processing systems. This constitutes a perfect scenario for the International Reference Ionosphere (IRI) to assimilate this huge new database and to satisfy the new needs of the aeronomic community: an IRI with meteorological capability. The first step before the implementation of an assimilative procedure is to validate the new data. This work intends to contribute in this direction by studying the differences (systematic and statistical) between the F2 peak parameters (hmF2 and NmF2) predicted by the IRI(CCIR) and those obtained from the electron density profiles computed with LPIM-COSMIC/Formosat3 (LPIM-C/F3) technique. The analyzed period extends from January 2007 to October 2012, thus covering all the different seasonal Sun–Earth configurations and a range of solar activity going from low to mid-high level. The analysis shows that there is no significant systematic bias between the IRI and LPIM-C/F3 values on both parameters. The obtained differences are comparable to those found between IRI and other models and data sources. In addition a correlation with the solar activity level is observed. The analysis performed is also helpful to study and asses the potentiality of the meteorological information contained in the LPIM-C/F3 by analyzing the standard deviation of the differences. This extra information could represent the key element to improve the IRI predicting capabilities.
Fil: Azpilicueta, Francisco Javier. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Altadill, D.. Universitat Ramon Llull; España
Fil: Brunini, Claudio Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Torta, J. M.. Universitat Ramon Llull; España
Fil: Blanch, Eva Valeria. Universitat Ramon Llull; España
description During the last decade the amount of ionosphere measurements, from ground and space born sources, has substantially increased along with the development of high end processing systems. This constitutes a perfect scenario for the International Reference Ionosphere (IRI) to assimilate this huge new database and to satisfy the new needs of the aeronomic community: an IRI with meteorological capability. The first step before the implementation of an assimilative procedure is to validate the new data. This work intends to contribute in this direction by studying the differences (systematic and statistical) between the F2 peak parameters (hmF2 and NmF2) predicted by the IRI(CCIR) and those obtained from the electron density profiles computed with LPIM-COSMIC/Formosat3 (LPIM-C/F3) technique. The analyzed period extends from January 2007 to October 2012, thus covering all the different seasonal Sun–Earth configurations and a range of solar activity going from low to mid-high level. The analysis shows that there is no significant systematic bias between the IRI and LPIM-C/F3 values on both parameters. The obtained differences are comparable to those found between IRI and other models and data sources. In addition a correlation with the solar activity level is observed. The analysis performed is also helpful to study and asses the potentiality of the meteorological information contained in the LPIM-C/F3 by analyzing the standard deviation of the differences. This extra information could represent the key element to improve the IRI predicting capabilities.
publishDate 2014
dc.date.none.fl_str_mv 2014-07
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/11336/32565
Torta, J. M.; Blanch, Eva Valeria; Azpilicueta, Francisco Javier; Altadill, D.; Brunini, Claudio Antonio; A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR); Elsevier; Advances in Space Research; 55; 8; 7-2014; 2012-2019
0273-1177
CONICET Digital
CONICET
url http://hdl.handle.net/11336/32565
identifier_str_mv Torta, J. M.; Blanch, Eva Valeria; Azpilicueta, Francisco Javier; Altadill, D.; Brunini, Claudio Antonio; A comparison of the LPIM-COSMIC F2 peak parameters determinations against the IRI(CCIR); Elsevier; Advances in Space Research; 55; 8; 7-2014; 2012-2019
0273-1177
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.asr.2014.08.008
info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0273117714005201
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
application/pdf
dc.publisher.none.fl_str_mv Elsevier
publisher.none.fl_str_mv Elsevier
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 13.22299

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