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Reference TypeJournal Article
Identifier8JMKD3MGP3W/3UGDGGL
Repositorysid.inpe.br/plutao/2019/12.03.17.36
Metadatasid.inpe.br/plutao/2019/12.03.17.36.06
Siteplutao.sid.inpe.br
DOI10.3847/1538-4357/ab40af
Labellattes: 2768849231719678 4 RodríguezGómezPalaVieiLago:2019:Pl&lEv
ISSN0004-637X
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Citation KeyRodríguezGómezPalaVieiLago:2019:PlEvTh
Author1 Rodríguez Gómez, Jenny Marcela
2 Palacios, Judith
3 Vieira, Luis Eduardo Antunes
4 Lago, Alisson Dal
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
2 Leibniz Institut für Sonnenphysik (KIS)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 J.RodriquezGomez@skoltech.ru
2
3 luis.vieira@inpe.br
4 alisson.dallago@inpe.br
TitleThe plasma B evolution through the solar corona during solar cycles 23 and 24
JournalThe Astrophysical Journal
Year2019
Volume884
Number1
KeywordsSun: magnetic fields – Sun: photosphere.
AbstractThe plasma β 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 β variations through the solar corona during solar cycles 23 and 24. The plasma β 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 β 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 Re). In the photosphere we use temperature values from the FALC model to obtain plasma β in QS and faculae. Additionally, variations of the magnetic and kinetic pressure were modeled during the last solar cycles at coronal heights.
Pages88-95
Languagept
Type of Workjournal article
Secondary TypePRE PI
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX; SCOPUS.
AreaCEA
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
Size1568 KiB
Number of Files1
Target Filerodriguez_plasma.pdf
Last Update2019:12.06.09.58.11 dpi.inpe.br/plutao@80/2008/08.19.15.01 lattes
Metadata Last Update2019:12.09.20.33.47 dpi.inpe.br/plutao@80/2008/08.19.15.01 administrator {D 2019}
Document Stagecompleted
Is the master or a copy?is the master
Mirrorsid.inpe.br/mtc-m19/2013/05.22.12.17
e-Mail (login)self-uploading-INPE-MCTI-GOV-BR
Reader Groupadministrator
lattes
Visibilityshown
Transferable1
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
Content TypeExternal Contribution
Document Stagenot transferred
Version Typepublisher
Archiving Policyallowpublisher allowfinaldraft
Next Higher Units8JMKD3MGPCW/3EU29DP
source Directory Contentthere are no files
agreement Directory Contentthere are no files
History2019-12-03 17:36:55 :: lattes -> administrator :: 2019
2019-12-04 14:42:57 :: administrator -> lattes :: 2019
2019-12-06 09:58:12 :: lattes -> administrator :: 2019
2019-12-09 20:33:47 :: administrator -> self-uploading-INPE-MCTI-GOV-BR :: 2019
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission rightsholder secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url usergroup
Access Date2019, Dec. 10
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