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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/MTC-m13@80/2005/12.02.18.30
Last Update2006:06.14.04.44.36 (UTC) administrator
Metadata Repositorysid.inpe.br/MTC-m13@80/2005/12.02.18.30.16
Metadata Last Update2018:06.04.04.12.30 (UTC) administrator
Secondary KeyINPE-12223-PRE/7557
Citation KeySavianDSLSSBSAEVGMBS:2005:SoInOr
TitleOn the solar and interplanetary origin of intense geomagnetic storms and ground cosmic ray response
FormatOn-line
ProjectMAGHEL: Magnetosfera e Heliosfera
Year2005
Access Date2024, Apr. 23
Secondary TypePRE CI
Number of Files1
Size295 KiB
2. Context
Author 1 Savian, Jairo F.
 2 Dal lago, Alisson
 3 Silva, Marlos Rockenbach da
 4 Lucas, Aline de
 5 Santos, Luiz C.
 6 Silva, Samuel M. da
 7 Braga, Carlos R.
 8 Silva, Cristian W. S. da
 9 Andrioli, Vânia F.
10 Echer, Ezequiel
11 Vieira, Luis Eduardo
12 Gonzalez Alarcon, Walter Demétrio
13 Munakata, Kazuoki
14 Bieber, John
15 Schuch, Nelson Jorge
Resume Identifier 1
 2 8JMKD3MGP5W/3C9JGH3
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10 8JMKD3MGP5W/3C9JH3D
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15 8JMKD3MGP5W/3C9JHUD
Group 1
 2 DGE-INPE-MCT-BR
 3 DGE-INPE-MCT-BR
 4 DGE-INPE-MCT-BR
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10 DGE-INPE-MCT-BR
11 DGE-INPE-MCT-BR
12 DGE-INPE-MCT-BR
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15 RSU-INPE-MCT-BR
Affiliation 1 Universidade Federal de Santa Maria (UFSM)
 2 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
 3 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
 4 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
 5 Universidade Federal de Santa Maria (UFSM)
 6 Universidade Federal de Santa Maria (UFSM)
 7 Universidade Federal de Santa Maria (UFSM)
 8 Universidade Federal de Santa Maria (UFSM)
 9 Universidade Federal de Santa Maria (UFSM)
10 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
11 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
12 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
13 Shinshu University, Faculty of Sciences, Physics Department
14 University of Delawere, Bartol Research Institute
15 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference NameEl Leoncito School on Solar Physics.
Conference LocationSan Juan
Date28 nov.- 5 dez.
Book TitleProceedings
History (UTC)2005-12-07 17:06:30 :: seeger05 -> jeferson ::
2006-01-18 17:29:38 :: jeferson -> jefferson ::
2006-01-18 17:31:14 :: jefferson -> marciana ::
2006-07-19 21:45:20 :: marciana -> administrator ::
2006-09-27 20:14:58 :: administrator -> marciana ::
2008-05-02 14:59:04 :: marciana -> administrator ::
2018-06-04 04:12:30 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
KeywordsSPACE GEOPHYSICS
Solar origin
Interplanetary origin
Magnetic storms
Cosmic ray
GEOFÍSICA ESPACIAL
Origem solar
Origem interplanetária
Tempestades magnéticas
Raios cósmicos
AbstractGeomagnetic Storms are episodes of extraordinary fluctuation of the Terrestrial Magnetic Field (Gonzalez et al., 1994). It is believed that the physical mechanism responsible for the transfer of energy from the Solar Wind to the Magnetosphere is the reconnection between the Interplanetary Magnetic Field and the Terrestrial Magnetic Field (Tsurutani and Gonzalez, 1997). For the occurrence of such a mechanism, it is necessary that the Interplanetary Magnetic Field possesses substantial component in the negative Z direction considering the system of coordinates Sun-Magnetosphere, or Bs, South. The present work has as objective to identify the types of interplanetary structures that caused the Geomagnetic storms during period close to the maximum of the Solar Cycle 23, from 2002 to 2003. During this period there were observations of cosmic rays from the International Muon Detector Network, of which the Southern Space Observatory-SSO (OES/CRSPE/INPE) started to participate since 2001. These observations are being used for the forecasting of the occurrence of these Geomagnetic Storm with high efficiency, up to 8 hours in advance of alert (Munakata et al., 2000). The identification of the interplanetary structures that caused intense storms in this period is very important for a future comparison with the observations of cosmic rays (muons), allowing the verification wheter there is some preferential type of structure that can be detected by the muon detector network.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > On the solar...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > On the solar...
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/MTC-m13@80/2005/12.02.18.30
zipped data URLhttp://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/12.02.18.30
Languageen
Target Fileon the solar.pdf
User Groupadministrator
seeger05
marciana
administrator
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.39.46 1
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 1
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber contenttype copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress identifier isbn issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
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