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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/42EDFKP
Repositorysid.inpe.br/mtc-m21c/2020/05.05.11.59   (restricted access)
Last Update2020:05.05.11.59.36 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/05.05.11.59.36
Metadata Last Update2022:01.04.01.35.07 (UTC) administrator
DOI10.1016/j.asr.2020.02.025
ISSN0273-1177
1879-1948
Citation KeyMachoCorPauAngVie:2020:IoReJu
TitleIonospheric response to the June 2015 geomagnetic storm in the South American region
Year2020
MonthMay
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4155 KiB
2. Context
Author1 Macho, Eduardo Perez
2 Correia, Emília
3 Paulo, Claudio Machado
4 Angulo, Lady
5 Vieira, José Augusto Gomes
Resume Identifier1
2 8JMKD3MGP5W/3C9JH2C
Group1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Presbiteriana Mackenzie
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Presbiteriana Mackenzie
4 Universidade Presbiteriana Mackenzie
5 Universidade Presbiteriana Mackenzie
Author e-Mail Address1 edu_point@hotmail.com
2 emilia.correia@inpe.br
JournalAdvances in Space Research
Volume65
Number9
Pages2172-2183
Secondary MarkB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I
History (UTC)2020-05-05 11:59:36 :: simone -> administrator ::
2020-05-05 11:59:37 :: administrator -> simone :: 2020
2020-05-05 12:00:01 :: simone -> administrator :: 2020
2022-01-04 01:35:07 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
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Transferable1
Content TypeExternal Contribution
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AbstractThe ionospheric dynamics in the South America (SA) sector during geomagnetic disturbed period from 21 to 24 June 2015 is investigated through ground ionosonde stations and Global Navigation Satellite System (GNSS) receivers, supported by Very Low Frequency (VLF) and magnetometer data. These disturbances were caused by 3 interplanetary shocks (IS) derived from 3 consecutives coronal mass ejections (CME) from the same solar active region; the first two CME were caused by filament eruptions, and the third was a much larger full halo CME, associated with a M2.6 solar flare. The first 2 shocks were compressive and did not cause an immediate response to the ionosphere in the analyzed region, while the third shock increased considerably the electron density from low to high-latitudes, triggering the second strongest geomagnetic storm of the 24th solar cycle. It was possible to observe the expansion of the crest of equatorial ionospheric anomaly (EIA) at midlatitudes and high-latitudes mainly due to prompt penetration electric field (PPEF) during the main phase and the recovery phase of the geomagnetic storm during the day.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Ionospheric response to...
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4. Conditions of access and use
Languageen
Target Filemacho_ionosopheric.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
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Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 3
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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