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dc.contributor.author
Ezquer, Rodolfo Gerardo  
dc.contributor.author
Scida, Luis Alberto  
dc.contributor.author
Migoya Orue, Yenca Olivia  
dc.contributor.author
Nava, B.  
dc.contributor.author
Cabrera, Miguel Angel  
dc.contributor.author
Brunini, Claudio Antonio  
dc.date.available
2019-08-12T12:27:58Z  
dc.date.issued
2018-04  
dc.identifier.citation
Ezquer, Rodolfo Gerardo; Scida, Luis Alberto; Migoya Orue, Yenca Olivia; Nava, B.; Cabrera, Miguel Angel; et al.; NeQuick 2 and IRI Plas VTEC predictions for low latitude and South American sector; Elsevier; Advances in Space Research; 61; 7; 4-2018; 1803-1818  
dc.identifier.issn
0273-1177  
dc.identifier.uri
http://hdl.handle.net/11336/81388  
dc.description.abstract
Using vertical total electron content (VTEC) measurements obtained from GPS satellite signals the capability of the NeQuick 2 and IRI Plas models to predict VTEC over the low latitude and South American sector is analyzed. In the present work both models were used to calculate VTEC up to the height of GPS satellites. Also, comparisons between the performance of IRI Plas and IRI 2007 have been done. The data correspond to June solstice and September equinox 1999 (high solar activity) and they were obtained at nine stations. The considered latitude range extends from 18.4°N to −64.7°N and the longitude ranges from 281.3°E to 295.9°E in the South American sector. The greatest discrepancies among model predictions and the measured VTEC are obtained at low latitudes stations placed in the equatorial anomaly region. Underestimations as strong as 40 TECU [1 TECU = 1016 m−2] can be observed at BOGT station for September equinox, when NeQuick2 model is used. The obtained results also show that: (a) for June solstice, in general the performance of IRI Plas for low latitude stations is better than that of NeQuick2 and, vice versa, for highest latitudes the performance of NeQuick2 is better than that of IRI Plas. For the stations TUCU and SANT both models have good performance; (b) for September equinox the performances of the models do not follow a clearly defined pattern as in the other season. However, it can be seen that for the region placed between the Northern peak and the valley of the equatorial anomaly, in general, the performance of IRI Plas is better than that of NeQuick2 for hours of maximum ionization. From TUCU to the South, the best TEC predictions are given by NeQuick2. The source of the observed deviations of the models has been explored in terms of CCIR foF2 determination in the available ionosonde stations in the region. Discrepancies can be also related to an unrealistic shape of the vertical electron density profile and or an erroneous prediction of the plasmaspheric contribution to the vertical total electron content. Moreover, the results of this study could be suggesting that in the case of NeQuick, the underestimation trend could be due to the lack of a proper plasmaspheric model in its topside representation. In contrast, the plasmaspheric model included in IRI, leads to clear overestimations of GPS derived TEC.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Elsevier  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Iri Plas Model  
dc.subject
Nequick 2 Model  
dc.subject
Vertical Total Electron Content  
dc.subject.classification
Meteorología y Ciencias Atmosféricas  
dc.subject.classification
Ciencias de la Tierra y relacionadas con el Medio Ambiente  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
NeQuick 2 and IRI Plas VTEC predictions for low latitude and South American sector  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2019-08-07T14:06:42Z  
dc.journal.volume
61  
dc.journal.number
7  
dc.journal.pagination
1803-1818  
dc.journal.pais
Países Bajos  
dc.journal.ciudad
Amsterdam  
dc.description.fil
Fil: Ezquer, Rodolfo Gerardo. Universidad Tecnológica Nacional; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina  
dc.description.fil
Fil: Scida, Luis Alberto. Universidad Nacional de Tucumán; Argentina  
dc.description.fil
Fil: Migoya Orue, Yenca Olivia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina  
dc.description.fil
Fil: Nava, B.. Universidad Nacional de Tucumán; Argentina  
dc.description.fil
Fil: Cabrera, Miguel Angel. Universidad Tecnológica Nacional; Argentina  
dc.description.fil
Fil: Brunini, Claudio Antonio. The Abdus Salam. International Centre for Theoretical Physics; Italia. Universidad Nacional de La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina  
dc.journal.title
Advances in Space Research  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S027311771730724X?via%3Dihub  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1016/j.asr.2017.10.003