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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3APEQ48
Repositorysid.inpe.br/mtc-m19/2011/11.09.17.25   (restricted access)
Last Update2011:11.09.17.33.40 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/11.09.17.25.56
Metadata Last Update2021:07.18.04.02.13 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.jastp.2011.01.010
ISSN1364-6826
Citation KeyCostaDomiMendBrum:2011:CaSt
TitleInterplanetary medium condition effects in the South Atlantic Magnetic Anomaly: A case study
Year2011
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size956 KiB
2. Context
Author1 Costa, Aracy Mendes da
2 Domingues, Margarete Oliveira
3 Mendes Junior, Odim
4 Brum, Christiano Garnett Marques
Resume Identifier1
2 8JMKD3MGP5W/3C9JHQP
3 8JMKD3MGP5W/3C9JJ28
Group1 DGE-CEA-INPE-MCT-BR
2 LAC-CTE-INPE-MCT-BR
3 DGE-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Natl Astron & Ionosphere Ctr, Space & Atmospher Sci Dept, Arecibo Observ, Arecibo, PR USA
Author e-Mail Address1 aracy@dge.inpe.br
2 margarete@lac.inpe.br
3 odim@dge.inpe.br
e-Mail Addresstereza@sid.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume73
Number11-12
Pages1478-1491
History (UTC)2011-12-27 15:23:56 :: valdirene -> administrator :: 2011
2012-07-15 03:00:01 :: administrator -> tereza@sid.inpe.br :: 2011
2012-08-15 12:42:57 :: tereza@sid.inpe.br -> banon :: 2011
2012-09-24 17:20:59 :: banon -> administrator :: 2011
2021-07-18 04:02:13 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsspace electrodynamics
south atlantic magnetic anomaly
solar energetic particles
wavelet
space weather keywords plus: solar-proton events
energetic electron-precipitation
polar-cap absorption
geomagnetic storm
equatorial ionosphere
model simulations
forbush decreases
particle events
space-weather
cosmic-rays
AbstractOne way to investigate the magnetosphere-ionosphere coupling is through the simultaneous observation of different parameters measured at different locations of the geospace environment and try to determine some relationships among them. The main objective of this work is to examine how the solar energetic particles and the interplanetary medium conditions may affect the space and time configuration of the ring current at low-latitudes and also to get a better understanding on how these particles interfere with the lower ionosphere in the South Atlantic Magnetic Anomaly region (SAMA). To accomplish this, the cosmic noise absorption (CNA) and the horizontal component of the Earth's magnetic field data measured from sites located in the SAMA region were compared with the proton and electron fluxes, interplanetary medium conditions (solar wind and the north-south component of the interplanetary magnetic field measured on board satellites), the SYM-H index and magnetometer data from Kakioka (KAK-Japan), located significantly outside the SAMA region. The time series analyzed correspond to the geomagnetic disturbance that occurred on August 25-30, 1998. The analysis was performed by implementing wavelet techniques, with particular attention to singularities detection, which highlights the presence of transient signals. The results are discussed in terms of the first three wavelet decomposition levels of the parameters. The magnitude of wavelet coefficients of the solar wind and proton flux at the two energy ranges analyzed is timely well correlated, indicating that these two signals are energetically linked. The larger wavelet coefficient amplitude of KAK and VSS magnetograms shows time delays that are compatible with an asymmetric configuration of the ring current, considering that at the storm time, VSS was at the dawn sector of the magnetosphere and KAK at the dusk side. The wavelet analysis of CNA signals reveals that the signal may be sensitive to the ionization produced by energetic electrons and protons as well. The time delays observed in wavelet coefficients may give an indication of the different accelerating process to which the particles are submitted when traveling along the magnetic field lines, from higher to lower latitudes, and the likely contribution of these particles to the ionization measured as an absorption of the cosmic noise in the lower ionosphere.
AreaCOMP
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4. Conditions of access and use
Languageen
Target FileCosta_interplanetary.pdf
User Groupadministrator
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Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/bibdigital/2013/09.22.23.14 3
sid.inpe.br/mtc-m21/2012/07.13.14.57.24 1
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn label lineage mark 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)tereza@sid.inpe.br
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