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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3Q9K49E
Repositorysid.inpe.br/mtc-m21b/2017/12.27.15.20
Last Update2021:02.26.13.18.06 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2017/12.27.15.20.21
Metadata Last Update2022:03.18.22.12.30 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyDalLagoBragMesqMend:2017:PrICPr
TitlePredicting ICME properties at 1AU
Year2017
Access Date2024, May 04
Secondary TypePRE CI
Number of Files1
Size68 KiB
2. Context
Author1 Dal Lago, Alisson
2 Braga, Carlos Roberto
3 Mesquita, Amanda Lucia
4 Mendonça, Rafael Rodrigues Souza de
Resume Identifier1 8JMKD3MGP5W/3C9JGH3
Group1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR
4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 alisson.dallago@inpe.br
2 carlos.braga@inpe.br
3 amanda.mesquita@inpe.br
4 rafael.mendonca@inpe.br
Conference NameAGU Fall Meeting
Conference LocationNew Orleans
Date11-15 Dec.
Book TitleProceedings
History (UTC)2017-12-27 15:20:21 :: simone -> administrator ::
2018-06-04 02:28:10 :: administrator -> simone :: 2017
2021-02-26 13:18:07 :: simone -> administrator :: 2017
2022-03-18 22:12:30 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractCoronal mass ejections (CMEs) are among the main origins of geomagnetic disturbances. They change the properties of the near-earth interplanetary medium, enhancing some key parameters, such as the southward interplanetary magnetic field and the solar wind speed. Both quantities are known to be related to the energy transfer from the solar wind to the Earths magnetosphere via the magnetic reconnection process. Many attempts have been made to predict the magnetic filed and the solar wind speed from coronagraph observations. However, we still have much to learn about the dynamic evolution of ICMEs as they propagate through the interplanetary space. Increased observation capability is probably needed. Among the several attempts to establish correlations between CME and ICME properties, it was found that the average CME propagation speed to 1AU is highly correlated to the ICME peak speed (Dal Lago et al, 2004). In this work, we present an extended study of such correlation, which confirms the results found in our previous study. Some suggestions on how to use this kind of results for space weather estimates are explored.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Predicting ICME properties...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Predicting ICME properties...
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source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34P/3Q9K49E
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34P/3Q9K49E
Languageen
Target Filedal lago_predicting.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 9
sid.inpe.br/bibdigital/2013/10.12.21.02 1
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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