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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/01.13.14.04
Last Update2004:03.29.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/01.13.14.04.57
Metadata Last Update2018:06.05.01.20.44 (UTC) administrator
Secondary KeyINPE-10359-PRE/5860
ISBN/ISSNISBN 85 88690-06-03
Citation KeyPadilhaAlvTriKitShi:2003:PiPuSo
TitlePiB pulsations at the South American equatorial zone during the 29 October 1994 magnetic storm
Year2003
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size189 KiB
2. Context
Author1 Padilha, Antonio Lopes
2 Alves, Maria Virgínia
3 Trivedi, Nalin Babulal
4 Kitamura, Tai-I
5 Shinohara, Manabu
Resume Identifier1 8JMKD3MGP5W/3C9JGJG
2 8JMKD3MGP5W/3C9JHRS
3 8JMKD3MGP5W/3C9JHTS
Group1 DGE-INPE-MCT-BR
2 LAP-INPE-MCT-BR
Conference NameInternational Congress of the Brazilian Geophysical Society, 8.
Conference LocationRio de Janeiro
Date14-19 Dec .2003
Book TitleProceedings
History (UTC)2018-06-05 01:20:44 :: administrator -> marciana :: 2003
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsfísica básica de plasma
AbstractThe effects of the great magnetic storm of 29 October 1994 on the daytime equatorial ionosphere have been studied by a ground-based array of fluxgate magnetometers in South America. The array covers around 2 h in magnetic local time and spans dip angles from 6.7oN to 10.8oS, with additional very-low latitude and nightside dip equator stations as reference. Following an abrupt increase in the AE index during the storm main phase, intense Pi1B activity is seen over a wide region around the prenoon dip equator. The pulsations are strongly attenuated not propagating outside the equatorial zone and have differences in time onset at different longitudes. It is proposed that they are associated with gradient-drift plasma instabilities triggered by prompt penetration of high latitude electric fields. Local ionospheric properties appear to control instability onset and growth rate along the dip equator. Figure 1 gives a map of South America with the locations of 11 stations. Also shown are relevant dip angles during the period of data acquisition indicating the dip equator
AreaFISPLASMA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAP > PiB pulsations at...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > PiB pulsations at...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/marciana/2004/01.13.14.04
zipped data URLhttp://urlib.net/zip/sid.inpe.br/marciana/2004/01.13.14.04
Languageen
Target FilePib.pdf
User Groupadministrator
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ET2RFS
8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.55.54 1
sid.inpe.br/mtc-m21/2012/07.13.14.56.48 1
sid.inpe.br/mtc-m21/2012/07.13.14.40.26 1
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsaffiliation archivingpolicy archivist callnumber copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
e-Mail (login)marciana
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