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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UM9CTS
Repositorysid.inpe.br/mtc-m21c/2020/01.02.13.07
Last Update2020:01.02.13.07.06 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2020/01.02.13.07.06
Metadata Last Update2022:03.18.22.11.31 (UTC) administrator
DOI10.1029/2019JA027187
ISSN2169-9402
Citation KeyBravoBatiSouzFopp:2019:IoReDi
TitleIonospheric response to disturbed winds during the 29 October 2003 geomagnetic storm in the brazilian sector
Year2019
MonthNov.
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size26796 KiB
2. Context
Author1 Bravo, Manuel Alejandro
2 Batisa, Inez Staciarini
3 Souza, Jonas Rodrigues de
4 Foppiano, A. J.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHFE
ORCID1 0000-0002-5648-429X
2 0000-0001-5385-4112
3
4 0000-0003-4374-538X
Group1 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidad de Concepción (UdeC)
Author e-Mail Address1 mbravo@dgeo.udec.cl
2 inez.batista@inpe.br
3 jonas.souza@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume124
Number11
Pages9405-9419
History (UTC)2020-01-02 13:07:06 :: simone -> administrator ::
2020-01-02 13:07:06 :: administrator -> simone :: 2019
2020-01-02 13:07:46 :: simone -> administrator :: 2019
2022-03-18 22:11:31 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractModeling the ionosphere during disturbed periods is one of the most challenging tasks due to the complexity of the phenomena that affect the electric fields and the whole thermosphere environment. It is well known that both, prompt penetration electric fields and large amounts of energy deposited in the polar region during disturbed periods, produce significant disturbances in the global electron density distribution, in particular, in the equatorial ionization anomaly development. Besides, the disturbance dynamo, traveling atmospheric disturbances, and traveling ionospheric disturbances also affect the equatorial ionization anomaly density distribution. In this work we use the Sheffield University Plasmasphere-Ionosphere Model at Instituto Nacional de Pesquisas Espaciais, to simulate the drastic effects that were observed at the low-latitude ionosphere in the Brazilian region during a very intense magnetic storm event, the so-called 2003 Halloween storms. In the absence of measured vertical drift during the storm, a new vertical drift deduced from the interplanetary electric field combined with the time variation of the F region virtual height is used as input. The simulation results showed that, in the case of the disturbed thermospheric wind, the ionospheric observations are better explained when a novel traveling wave-like disturbance propagating from north to south, at a velocity equal to 300 m/s, is considered.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Ionospheric response to...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Ionospheric response to...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3UM9CTS
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3UM9CTS
Languageen
Target Filebravo_ionospheric.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 3
sid.inpe.br/mtc-m21/2012/07.13.14.51.12 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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