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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3SB3S2H
Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.07
Last Update2019:01.08.15.31.28 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.07.32
Metadata Last Update2019:01.14.17.06.39 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBragaVoDaMeEcBaKw:2018:KiMeCo
TitleWhat causes CME travel time estimation errors: their kinematic measurements in the corona or the limited understanding of the forces in their IP propagation?
Year2018
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size139 KiB
2. Context
Author1 Braga, Carlos Roberto
2 Vourlidas, Angelos
3 Dal Lago, Alisson
4 Mendonça, Rafael Rodrigues Souza de
5 Echer, Ezequiel
6 Balmaceda, Laura
7 Kwon, Ryun Young
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGH3
4
5 8JMKD3MGP5W/3C9JH3D
Group1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
2
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
4
5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Johns Hopkins University Applied Physics Laboratory
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Chinese Academy of Sciences
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 George Mason University
7 George Mason University Fairfax
Author e-Mail Address1 carlos.braga@inpe.br
2
3 alisson.dallago@inpe.br
4
5 ezequiel.echer@inpe.br
Conference NameAGU Fall Meeting
Conference LocationWashington, D. C.
Date10-14 dec.
History (UTC)2018-12-03 15:07:32 :: simone -> administrator ::
2019-01-14 17:06:39 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe coronal mass ejections (CME) time-of-arrival (ToA) estimates from the corona to 1 AU have been a topic of central interest due to the space weather phenomena associated with their arrival, such as intense geomagnetic storms. Several ToA estimates using kinematic input from white-light coronagraphs observations, both from a single and multi-viewpoint, have been made available, especially in the last decade. Despite of the development of many methods, ToA estimates errors are no better than 10 hours, on average. Our objective is to evaluate whether these discrepancies are associated with the limited analytical description of the forces acting on CMEs or with the improper kinematic input from observations. We took a set of well-observed CMEs from the Sun to 1 AU and investigate possible reasons for the discrepancies. We considered that the CME propagation is controlled by the aerodynamic drag due to the background solar wind and the Lorentz forces. We discuss the discrepancies caused in the travel time estimate due to drag force in CMEs whose background solar wind conditions (such as speed) change dramatically in the period from the CME release until its arrival at 1 AU. We also estimate a possible force associated with the interaction of CMEs with interplanetary structures such as corotating interaction regions. Back-of-the-envelope calculations suggest that typical magnetic field and particle density observed in these structures could significantly change the CME velocity and lead to ToA errors. (This work is funded by FAPESP, Sao Paulo Research Foundation, grant #2017/21270-7).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > What causes CME...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 03/12/2018 13:07 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3SB3S2H
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3SB3S2H
Languageen
Target Fileabstract_carlos_agu_2018.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 3
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords 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 tertiarytype type url versiontype volume
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