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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3TKKK2H
Repositorysid.inpe.br/mtc-m21c/2019/07.10.11.58
Metadata Repositorysid.inpe.br/mtc-m21c/2019/07.10.11.58.05
Metadata Last Update2020:01.06.11.42.16 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBatistaSaSoAbBrBa:2019:MoLoLa
TitleModelling the low latitude ionosphere response to magnetic disturbances
Year2019
Access Date2024, May 16
Secondary TypePRE CI
2. Context
Author1 Batista, Inez Staciarini
2 Santos, A. M.
3 Souza, Jonas Rodrigues de
4 Abdu, Mangalathayil Ali
5 Bravo, M.
6 Bailey, G.
Resume Identifier1 8JMKD3MGP5W/3C9JHDA
2
3 8JMKD3MGP5W/3C9JHFE
4 8JMKD3MGP5W/3C9JHNK
Group1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
2
3 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
4 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 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidad de Concepción
6 Sheffield University
Author e-Mail Address1 inez.batista@inpe.br
2
3 jonas.souza@inpe.br
4 ma.abdu@inpe.br
Conference NameIUGG General Assembly, 27
Conference LocationMontréal, Canada
Date08-18 July
History (UTC)2019-07-10 11:58:06 :: simone -> administrator ::
2020-01-06 11:42:16 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe space weather events originated in the Sun can affect the whole thermosphere-ionosphere system at all latitudes. During such events disturbance electric fields (undershielding or overshielding) can penetrate from high to low latitudes causing significant disturbances in the electron density distribution and in the equatorial ionization anomaly (EIA) development. Besides that, the large amount of energy deposited in the polar region during disturbed periods will be responsible for the generation of disturbed winds that will flow towards the equator where they produce a disturbance dynamo which also affects the EIA density distribution. The TIDs and TADs are also sources of disturbances that propagate at high velocity reaching the equator 2-3 hours after the beginning of the magnetic storm. Particle precipitation is an additional source of perturbation at high latitudes as well as at the South Atlantic Magnetic Anomaly, where the conductivity can be affected by the extra ionization. Modeling the ionosphere during such disturbed periods is one of the most challenging tasks due to the complexity of the phenomena that affect the thermosphere environment as a whole. In this work we use the Sheffield University Plasmasphere-Ionosphere Model at INPE (SUPIM-INPE), to simulate the effects that were observed at the low latitude ionosphere in the South America longitude sector during some magnetic storm event. For some storms a few models are tested for the disturbed electric field and for the disturbed wind. A particle precipitation model is included in SUPIM, in order to test the ionospheric response to the enhanced conductivity.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Modelling the low...
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Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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