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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3AFLCEK
Repositorydpi.inpe.br/plutao/2011/09.22.18.53.23   (restricted access)
Last Update2011:12.08.12.08.43 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/09.22.18.53.24
Metadata Last Update2018:06.05.00.01.28 (UTC) administrator
DOI10.1016/j.asr.2011.05.036
ISSN0273-1177
Labellattes: 1106857072073407 6 AbreuSaFaJeBiPi:2011:AnInOf
Citation KeyAbreuSaFaJeBiPi:2011:InIoRe
TitleAn investigation of ionospheric F region response in the Brazilian sector to the super geomagnetic storm of May 2005
Year2011
MonthOct
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size1673 KiB
2. Context
Author1 Abreu, A. J.
2 Sahai, Y.
3 Fagundes, P. R.
4 Jesus, R.
5 Bittencourt, J. A.
6 Pillat, Valdir Gil
Group1
2
3
4
5 DAE-CEA-INPE-MCT-BR
Affiliation1
2 Departamento de Física e Astronomia, Universidade do Vale do Paraíba (UNIVAP), Av. Shishima Hifumi, 2911, São José dos Campos, São Paulo, Brazil
3 Departamento de Física e Astronomia, Universidade do Vale do Paraíba (UNIVAP), Av. Shishima Hifumi, 2911, São José dos Campos, São Paulo, Brazil
4 Departamento de Física e Astronomia, Universidade do Vale do Paraíba (UNIVAP), Av. Shishima Hifumi, 2911, São José dos Campos, São Paulo, Brazil
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Departamento de Física e Astronomia, Universidade do Vale do Paraíba (UNIVAP), Av. Shishima Hifumi, 2911, São José dos Campos, São Paulo, Brazil
Author e-Mail Address1 abreu.alessandro@gmail.com
2 sahai@univap.br
3 fagundes@univap.br
4 jesus.rodolfo@hotmail.com
5 jabittencourt@hotmail.com
6 valdirgp@univap.br
e-Mail Addressvaldirgp@univap.br
JournalAdvances in Space Research
Volume48
Number7
Pages1211-1220
Secondary MarkB4_ASTRONOMIA_/_FÍSICA B3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS B1_INTERDISCIPLINAR
History (UTC)2011-09-23 14:11:19 :: lattes -> administrator :: 2011
2011-09-24 15:24:08 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2011-12-08 12:08:53 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2011-12-14 17:07:17 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2011-12-27 15:24:30 :: secretaria.cpa@dir.inpe.br -> tereza@sid.inpe.br :: 2011
2012-01-18 11:28:53 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 00:01:28 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGeomagnetic storm
Ionosphere
Equatorial ionospheric irregularities
AbstractIn this paper, we have investigated the responses of the ionospheric F region at equatorial and low latitude regions in the Brazilian sector during the super geomagnetic storm on 15-16 May 2005. The geomagnetic storm reached a minimum Dst of -263 nT at 0900 UT on 15 May. In this paper, we present vertical total electron content (vTEC) and phase fluctuations (in TECU/min) from Global Positioning System (GPS) observations obtained at Belem, Brasilia, Presidente Prudente, and Porto Alegre, Brazil, during the period 14-17 May 2005. Also, we present ionospheric parameters h'F, hpF2, and foF2, using the Canadian Advanced Digital Ionosonde (CADI) obtained at Palmas and Sao Jose dos Campos, Brazil, for the same period. The super geomagnetic storm has fast decrease in the Dst index soon after SSC at 0239 UT on 15 May. It is a good possibility of prompt penetration of electric field of magnetospheric origin resulting in uplifting of the F region. The vTEC observations show a trough at BELE and a crest above UEPP, soon after SSC, indicating strengthening of nighttime equatorial anomaly. During the daytime on 15 and 16 May, in the recovery phase, the variations in foF2 at SJC and the vTEC observations, particularly at BRAZ, UEPP, and POAL, show large positive ionospheric storm. There is ESF on the all nights at PAL, in the post-midnight (UT) sector, and phase fluctuations only on the night of 14-15 May at BRAZ, after the SSC. No phase fluctuations are observed at the equatorial station BELE and low latitude stations (BRAZ, UEPP, and POAL) at all other times. This indicates that the plasma bubbles are generated and confined on this magnetically disturbed night only up to the low magnetic latitude and drifted possibly to west.
AreaFISMAT
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > An investigation of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileAbreu-AdvSpaceRes-v48-n7-p1211-1220-science[1].pdf
User Groupadministrator
lattes
secretaria.cpa@dir.inpe.br
tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)tereza@sid.inpe.br
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