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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/iris@1916/2006/03.09.16.37   (restricted access)
Last Update2006:03.24.12.14.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2006/03.09.16.37.42
Metadata Last Update2018:06.05.01.16.44 (UTC) administrator
Secondary KeyINPE-13584-PRE/8794
ISSN0273-1177
Citation KeyTrivediPatSchBarDut:2005:GePhSo
TitleGeomagnetic phenomena in the south atlantic anomaly region in Brazil
Year2005
Access Date2024, May 18
Secondary TypePRE PI
Number of Files1
Size152 KiB
2. Context
Author1 Trivedi, Nalin Babulal
2 Pathan, B. M.
3 Schuch, Nelson Jorge
4 Barreto, M.
5 Dutra, Luciano Vieira
Resume Identifier1 8JMKD3MGP5W/3C9JHTS
2
3 8JMKD3MGP5W/3C9JHUD
4
5 8JMKD3MGP5W/3C9JHMA
Group1 RSU-INPE-MCT-BR
2 DPI-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, RSU
2 Instituto Nacional de Pesquisas Espaciais, DPI
JournalAdvances in Space Research
Volume36
Number10
Pages2021-2024
History (UTC)2006-03-24 12:14:48 :: jefferson -> administrator ::
2012-07-17 12:41:50 :: administrator -> jefferson ::
2012-10-03 14:52:31 :: jefferson -> administrator :: 2005
2018-06-05 01:16:44 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGeomagnetic phenomena
south atlantic anomaly
south atlantic anomaly in Brazil
geomagnatic phenomena in Brazil
AbstractThe secular variation in the total geomagnetic field F and the westward drift of South Atlantic magnetic anomaly (SAMA) observed in Brazil during the 20th century are presented. According to the International Geomagnetic Reference Field (IGRF) model for the years 2000 to 2005 the present value of F at São Martinho da Serra (29°.43 S, 53°.80 W) is 22,883 nT, a value close to the measured one. The secular variation in F at this station is −28 nT per year. It is difficult to forecast the drift movement of this anomaly (SAMA) in the coming years, however, it should be a matter of concern should the field continue to decrease at the present rate or even faster. We have also noted that both continuous and impulsive pulsations observed in the H component of the geomagnetic field at São Martinho da Serra are enhanced due to the particle precipitations in the SAMA region. We present here few events observed at São Martinho da Serra showing clear enhancement of the amplitudes of pulsation and discuss the processes for electron precipitation in the atmosphere above SAMA. This justifies the need of a magnetic observatory at São Martinho da Serra not only to monitor the westward drift of the SAMA but also to provide valuable observations for the Space Weather studies at our institute.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDPI > Geomagnetic phenomena in...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Geomagnetic phenomena in...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filetrivedi.pdf
User Groupadministrator
jefferson
Reader Groupadministrator
jefferson
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EQCCU5
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.53.50 1
sid.inpe.br/mtc-m21/2012/07.13.14.57.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.56.48 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format identifier isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
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