1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/44CP2BE |
Repository | sid.inpe.br/mtc-m21c/2021/03.23.12.20 |
Metadata Repository | sid.inpe.br/mtc-m21c/2021/03.23.12.20.47 |
Metadata Last Update | 2022:04.03.19.25.05 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | NogueiraPicBarDenBat:2021:LaDeIo |
Title | Latitudinal dependence of the ionspheric response to solar flare |
Year | 2021 |
Access Date | 2024, May 18 |
Secondary Type | PRE CN |
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2. Context | |
Author | 1 Nogueira, P. A. B. 2 Picanço, Giorgio Arlan da Silva 3 Barbosa Neto, Paulo França 4 Denardini, Clezio Marcos 5 Batista, Paulo Prado |
Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JJ3H |
Group | 1 2 DIHPA-CGCE-INPE-MCTI-GOV-BR 3 4 DIHPA-CGCE-INPE-MCTI-GOV-BR 5 DIHPA-CGCE-INPE-MCTI-GOV-BR |
Affiliation | 1 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 Address | 1 2 giorgiopicanco@gmail.com 3 cristiano.wrasse@inpe.br 4 clezio.denardin@inpe.br 5 paulopradobatista@yahoo.com |
Conference Name | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA) |
Conference Location | Online |
Date | 22-26 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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Abstract | In 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Latitudinal dependence of... |
doc Directory Content | there are no files |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/46KTFK8 |
Host Collection | urlib.net/www/2017/11.22.19.04 |
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6. Notes | |
Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Description control | |
e-Mail (login) | simone |
update | |
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