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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZQjxQKY/Gt3nx
Repositorysid.inpe.br/ePrint@80/2005/06.15.12.31   (restricted access)
Last Update2005:06.15.12.31.15 (UTC) administrator
Metadata Repositorysid.inpe.br/ePrint@80/2005/06.15.12.31.16
Metadata Last Update2018:06.04.04.12.43 (UTC) administrator
Secondary KeyINPE-12559-PRE/7856
ISSN0103-9733
Citation KeyBalmacedaGESVDGG:2004:SoOrSu
TitleThe solar origins of the Sun-Earth connection events on april 1999 and february 2000
Year2004
Secondary Date2004
MonthDec.
Access Date2024, Apr. 28
Secondary TypePRE PN
Number of Files1
Size302 KiB
2. Context
Author1 Balmaceda, L. A.
2 Gonzales Alarcon, Walter Demétrio
3 Echer, Ezequiel
4 Santos, J. C.
5 Vieira, Luis Eduardo Antunes
6 Dal Lago, Alisson
7 Guarnieri, Fernando Luiz
8 Gonzalez, Alicia Luisa Clua de
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
4
5
6 8JMKD3MGP5W/3C9JGH3
Group1 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofisica Espacial(INPE, DGE)
2 Max Planck Inst Sonnensyst Forsch
JournalBrazilian Journal of Physics
Volume34
Number4b
Pages1745-1747
History (UTC)2010-05-14 01:58:01 :: alexandra -> administrator ::
2018-06-04 04:12:43 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractIn this work we present a comparison between the solar origins of two solar-terrestrial connection events occurring on April 1999 and February 2000, respectively. On April 13 (1999), a coronal mass ejection (CME) appeared for the first time in LASCO-C2 coronagraph field of view at 03:30 UT. The possible solar disc source of this CME was located at coordinates N25 E05, and it consisted on flaring activity together with a filament eruption as seen in EIT images. The geomagnetic storm with a Dst peak of -91 nT registered on April, 17 was attributed to this solar surface activity. On February 8, 9 and 10 (2000) three Earth-directed halo CMEs were recorded by LASCO coronagraphs. The interaction of two of them caused the intense interplanetary geomagnetic storm registered on February 12 (Dst = -110 nT). The CMEs detected on February 8 and 10 were launched from AR 8858 and the source of the activity was attributed to two solar flares of X-ray class M1.3 and C7.3 respectively. The CME detected on February 9 was originated in AR 8853 and flaring activity was also identified as the solar source for this event. In this study we discuss the solar origins of the events that gave rise to coronal and interplanetary disturbances and as a consequence produced geomagnetic activity at the Earth. This work is part of a complete study that is searching the solar origin, the interplanetary aspects and the magnetospheric effects of these events.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The solar origins...
doc Directory Contentaccess
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agreement Directory Contentthere are no files
4. Conditions of access and use
LanguageEnglish
Target Filesolar origins.pdf
User Groupadministrator
alexandra
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; SCIELO.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn keywords label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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