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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/32565
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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 Técnicas2025-09-29T10:35:22Zoai: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:34982025-09-29 10:35:22.599CONICET 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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1844614371694608384 |
score |
13.070432 |