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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/44CP2BE
Repositorysid.inpe.br/mtc-m21c/2021/03.23.12.20
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.23.12.20.47
Metadata Last Update2022:04.03.19.25.05 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyNogueiraPicBarDenBat:2021:LaDeIo
TitleLatitudinal dependence of the ionspheric response to solar flare
Year2021
Access Date2024, May 18
Secondary TypePRE CN
2. Context
Author1 Nogueira, P. A. B.
2 Picanço, Giorgio Arlan da Silva
3 Barbosa Neto, Paulo França
4 Denardini, Clezio Marcos
5 Batista, Paulo Prado
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JJ3H
Group1
2 DIHPA-CGCE-INPE-MCTI-GOV-BR
3
4 DIHPA-CGCE-INPE-MCTI-GOV-BR
5 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Federal Institute of Education, Science and Technology of S˜ao Paulo
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)
Author e-Mail Address1
2 giorgiopicanco@gmail.com
3 cristiano.wrasse@inpe.br
4 clezio.denardin@inpe.br
5 paulopradobatista@yahoo.com
Conference NameSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Conference LocationOnline
Date22-26 mar.
History (UTC)2021-03-23 12:20:47 :: simone -> administrator ::
2021-06-22 19:11:15 :: administrator -> simone :: 2021
2021-06-22 20:49:54 :: simone -> administrator :: 2021
2022-04-03 19:25:05 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractIn the present we study the ionospheric response for four X2- class intense solar flares that occurred in between 2014-2015, indeed we have used the GNSS receivers operating in South America to calculated a Total Electron Content Map (TECmap). By using the TECmap a disturbance ionospheric index (DIX) was developed, allowing the analyzes of the latitudinal dependence of the ionospheric disturbances. Preliminary results are indicating a local time and latitudinal dependence in the ionospheric response, showing that the largest disturbances occur nearby noon and at the locations of the Equatorial Ionization Anomaly crest. Finally, we compare the DIX response to solar flare and magnetic storms of different magnitudes. Both events, magnetic storms and solar flares, can have serious consequences to technological systems of public and private agencies around Brazilian sector. We believe this study can help to better understand the effects of solar flares in the ionosphere.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Latitudinal dependence of...
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Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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