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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3ULAHFP
Repositorysid.inpe.br/mtc-m21c/2019/12.27.15.53
Last Update2019:12.27.15.53.36 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/12.27.15.53.36
Metadata Last Update2019:12.27.23.17.32 (UTC) administrator
DOI10.3847/1538-4357/ab40af
ISSN0004-637X
1538-4357
Citation KeyRodríguezGómezPalaVieiDalL:2019:PlBeEv
TitleThe plasma beta evolution through the solar corona during solar cycles 23 and 24
Year2019
MonthOct.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1568 KiB
2. Context
Author1 Rodríguez Gómez, Jenny Marcela
2 Palacios, Judith
3 Vieira, Luis Eduardo Antunes
4 Dal Lago, Alisson
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JGH3
Group1
2
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Skolkovo Institute of Science and Technology (Skoltech)
2 Leibniz Institut für Sonnenphysik (KIS)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3 luis.vieira@inpe.br
4 alisson.dallago@inpe.br
JournalAstrophysical Journal
Volume884
Number1
Pagese88
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
History (UTC)2019-12-27 15:53:36 :: simone -> administrator ::
2019-12-27 15:53:37 :: administrator -> simone :: 2019
2019-12-27 15:55:37 :: simone -> administrator :: 2019
2019-12-27 23:17:32 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsSun: magnetic fields
Sun: photosphere
AbstractThe plasma beta is important in the investigation of interchanging roles of plasma and magnetic pressure in the solar atmosphere. It can help to describe features over the photosphere and their changes at different heights. The goal of this paper is to obtain the plasma beta variations through the solar corona during solar cycles 23 and 24. The plasma beta is reconstructed in different layers of the solar atmosphere. For this purpose, we use an updated version of the COronal DEnsity and Temperature model. In this version we selected different features in the solar atmosphere such as quiet-Sun (QS), faculae, and active regions. We calculate the beta variations at different layers in the solar corona (R = 1.14, 1.19, 1.23, 1.28, 1.34, 1.40, 1.46, 1.53, 1.61, 1.74, 1.79, 1.84, and 1.90 R-circle dot). In the photosphere we use temperature values from the FALC model to obtain plasma beta in QS and faculae. Additionally, variations of the magnetic and kinetic pressure were modeled during the last solar cycles at coronal heights.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The plasma beta...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 27/12/2019 12:53 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3ULAHFP
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3ULAHFP
Languageen
Target Filegomez_plasma.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.39.46 3
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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7. Description control
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