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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/2004/01.13.12.19
Last Update2004:03.29.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/01.13.12.19.18
Metadata Last Update2018:06.05.01.20.44 (UTC) administrator
Secondary KeyINPE-10363-PRE/5864
Citation KeyEcherAGGBSVDG:2003:InAs
TitleComparison between april 1999 and february 2000 solar-terrestrial connection events: interplanetary aspects
FormatOn-line
Year2003
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size452 KiB
2. Context
Author1 Echer, Ezequiel
2 Alves, Maria Virgínia
3 González-Alarcon, Walter Demétrio
4 Gonzalez-Alarcon, Alicia Luisa Clua de
5 Balmaceda, L. A.
6 Santos, C.
7 Vieira, Luiz Eduardo Antunes
8 Dal Lago, Alisson
9 Guarnieri, Fernando Luís
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
2 8JMKD3MGP5W/3C9JHRS
3
4
5
6
7
8 8JMKD3MGP5W/3C9JGH3
Group1 LAP-INPE-MCT-BR
2 DGE-INPE-MCT-BR
3 RSU-INPE-MCT-BR
Conference NameLatin American Workshop on Plasma Physics, 10; Brazilian Meeting on Plasma Physics, 7 (São Pedro, SP, Brazil, 2003).
Conference LocationSão Pedro, 2003
Date2003
Book TitleAnais
Tertiary TypePosters
History (UTC)2005-05-02 17:18:45 :: marciana -> administrator ::
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
geomagnetic storms
AbstractThe strong geomagnetic storms on April 17th 1999 (Dst peak = -91 nT) and on February 12th 2000 (Dst peak = -131 nT) were caused by different interplanetary structures. The April 1999 event was caused by a south-north fast magnetic cloud, which drove an interplanetary shock detected at 1 astronomical unit (UA) at 10:30 UT on April 16th 1999. This interplanetary shock had Alfvenic Mach number of about 2.5. The magnetic cloud arrived at UA around 23:00 UT on April 16th and ended around 19:00 UT on April 17th. The southward component of the interplanetary magnetic field remained above -10 nT for 5 hours, with peak value of -14 nT. The February 2000 event was caused by the interaction of two interplanetary remnants of coronal mass ejections. Two interplanetary shocks were detected on February 11th 2000 at 02:00 and at 23:00 UT. These shocks had Alfvenic Mach numbers of about 2.0 and 2.8, respectively, and were driven by interplanetary ejecta. The first interplanetary ejecta arrived at 1 UA around 16:00 UT on February 11th. However, it was engulfed by the second one around 20:00 UT on the same day, creating an intense and highly turbulent southward magnetic field, which remained above -10 nT for 3 hours, with peak value of -16 nT. In this paper the interplanetary aspects of these two solar-terrestrial connection events are analyzed and compared. Plasma and magnetic field data obtained from sensors on board ACE spacecraft orbiting L1 point are used.
AreaFISPLASMA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAP > Comparison between april...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Comparison between april...
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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/2004/01.13.12.19
zipped data URLhttp://urlib.net/zip/sid.inpe.br/marciana/2004/01.13.12.19
Languageen
Target Filecomparison.pdf
User Groupadministrator
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ET2RFS
8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
sid.inpe.br/bibdigital/2013/10.04.21.53 1
sid.inpe.br/bibdigital/2013/10.01.22.11 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 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 type url versiontype volume
7. Description control
e-Mail (login)marciana
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