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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UAR3D8
Repositorysid.inpe.br/mtc-m21c/2019/10.30.10.49   (restricted access)
Last Update2019:10.30.10.49.21 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/10.30.10.49.21
Metadata Last Update2020:02.10.16.58.46 (UTC) simone
DOI10.1016/j.asr.2019.09.005
ISSN0273-1177
1879-1948
Citation KeyKlippPSFCPAHKBJFBSW:2019:EvIoMo
TitleEvaluation of ionospheric models for Central and South Americas
Year2019
MonthNov.
Access Date2025, July 01
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4519 KiB
2. Context
Author 1 Klipp, Telmo dos Santos
 2 Petry, Adriano
 3 Souza, Jonas Rodrigues de
 4 Falcão, Gabriel Sandim
 5 Campos Velho, Haroldo Fraga de
 6 Paula, Eurico Rodrigues de
 7 Antreich, Felix
 8 Hoque, Mainul
 9 Kriegel, Martin
10 Berdermann, Jens
11 Jakowski, Norbert
12 Fernandez Gomez, Isabel
13 Borries, Claudia
14 Sato, Hiroatsu
15 Wilken, Volker
Resume Identifier 1
 2
 3 8JMKD3MGP5W/3C9JHFE
 4
 5 8JMKD3MGP5W/3C9JHC3
 6 8JMKD3MGP5W/3C9JH2U
Group 1 CRCRS-COCRE-INPE-MCTIC-GOV-BR
 2 CRCRS-COCRE-INPE-MCTIC-GOV-BR
 3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
 4 CRCRS-COCRE-INPE-MCTIC-GOV-BR
 5 LABAC-COCTE-INPE-MCTIC-GOV-BR
 6 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Tecnológico de Aeronáutica (ITA)
 8 German Aerospace Center (DLR)
 9 German Aerospace Center (DLR)
10 German Aerospace Center (DLR)
11 German Aerospace Center (DLR)
12 German Aerospace Center (DLR)
13 German Aerospace Center (DLR)
14 German Aerospace Center (DLR)
15 German Aerospace Center (DLR)
Author e-Mail Address 1 telmo.klipp@gmail.com
 2 adriano.petry@inpe.br
 3 jonas.souza@inpe.br
 4
 5 haroldo.camposvelho@inpe.br
 6 eurico.paula@inpe.br
 7 fean@ita.br
 8 Mainul.Hoque@dlr.de
 9 Martin.Kriegel@dlr.de
10 Jens.Berdermann@dlr.de
11 Norbert.Jakowski@dlr.de
12 Isabel.FernandezGomez@dlr.de
13 Claudia.Borries@dlr.de
14 Hiroatsu.Sato@dlr.de
15 Volker.Wilken@dlr.de
JournalAdvances in Space Research
Volume64
Number10
Pages2125-2136
Secondary MarkB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
History (UTC)2019-10-30 10:49:21 :: simone -> administrator ::
2019-10-30 10:50:51 :: administrator -> simone :: 2019
2019-10-30 10:52:00 :: simone -> administrator :: 2019
2020-01-06 11:42:23 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsIonosphere
Total electron content
Physics-based ionospheric model
Empirical ionospheric model
Seasonal variation
Statistical evaluation
AbstractThis work shows a 20-month statistical evaluation of different Total Electron Content (TEC) estimators for the Central and South America regions. The TEC provided by the International GNSS Service (IGS) in the area covered around the monitoring GNSS stations are used as reference values, and they are compared to TEC estimates from the physics-based (Sheffield University Plasmasphere Ionosphere Model-PIM) and the empirical (Neustrelitz TEC Model-Global-NTCM-GL) models. The mean TEC values show strong dependence on both solar activity and seasonal variation. A clear response was noticed for a period close to 27 days due to the mean solar rotation, as seen in the solar flux measurements. Consistently, the mean TEC values present an annual variation with maxima during December solstices for southern stations with geographic latitudes greater than 25 degrees S. Semi-annual dependence has been observed in TEC for the sector between +/- 25 degrees of geographical latitude but with modulations caused by fluctuation in the solar radiation. We observed a high correlation between solar radio flux F10.7 and NTCM-GL outputs. The fast increases in F10.7 index have caused significant differences between IGS data and NTCM-GL results mainly for equatorial and low latitudes. For the initial months of the evaluated period (January-April, 2016), the errors of the physics-based model were considerably larger, mainly near the equatorial ionization anomaly. The discrepancies observed in SUPIM results are mainly due to inputs of solar EUV flux. The EUVAC model has underestimated EUV flux between January and April, 2016, when the solar activity was moderated and Solar2000 model has overestimated such flux during low solar cycle period between May and August, 2017. In relation to IGS data, the two assessed models presented smaller differences during the June solstice season of 2016.
AreaCEA
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4. Conditions of access and use
Languageen
Target Fileklipp_evaluation.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
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Reader Groupadministrator
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Visibilityshown
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Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
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Next Higher Units8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/bibdigital/2013/09.22.23.14 - 10
sid.inpe.br/mtc-m21/2012/07.13.14.49.40 - 9
sid.inpe.br/bibdigital/2013/10.04.21.53 - 7
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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