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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UALKMP
Repositorysid.inpe.br/mtc-m21c/2019/10.29.10.47   (restricted access)
Last Update2019:10.29.10.47.47 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/10.29.10.47.47
Metadata Last Update2020:01.06.11.42.23 (UTC) administrator
DOI10.1007/s11207-019-1534-3
ISSN0038-0938
1573-093X
Citation KeySodréFernSantWras:2019:RaNoSt
TitleRadio noise storms and the connection with the reorganization of photospheric magnetic fields
Year2019
MonthOct.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2316 KiB
2. Context
Author1 Sodré, Zuleika A. L.
2 Fernandes, F. C. R.
3 Santos, Jean Carlo
4 Wrasse, Cristiano Max
ORCID1 0000-0003-4496-9051
2 0000-0003-2922-3358
3 0000-0003-1259-7230
4 0000-0001-8026-3625
Group1
2
3
4 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade do Vale do Paraíba (UNIVAP)
2 Universidade do Vale do Paraíba (UNIVAP)
3 Universidade Tecnológica Federal do Paraná (UTFPR)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 zuleika.sjc@bol.com.br
2
3
4 cristiano.wrasse@inpe.br
JournalSolar Physics
Volume294
Number10
Pagese140
Secondary MarkA2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO
History (UTC)2019-10-29 10:47:47 :: simone -> administrator ::
2019-10-29 10:47:47 :: administrator -> simone :: 2019
2019-10-29 10:48:52 :: simone -> administrator :: 2019
2020-01-06 11:42:23 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsRadio noise storms
Magnetic fields
Power spectra
SDO/HMI
e-CALLISTO
AbstractThis work presents the analysis of a Type-I radio noise storm (RNS) recorded by the CALLISTO spectrometers network. Considering that RNSs are associated with the reorganization of the photospheric magnetic field of active regions, we have analyzed the temporal evolution of the magnetic power spectra and the dissipation spectra of the photospheric magnetic field of two active regions (NOAA 11542 and NOAA 11543). This analysis was used to identify for which wave-numbers and time intervals this reorganization occurs. The Type-I emission is supposedly generated by the fundamental emission of plasma, and the reorganization of the line-of-sight component of the photospheric magnetic field was investigated as a possible mechanism responsible for the maintenance process of the RNS. The analysis of the magnetic power spectra and the dissipation spectra showed that the RNS was probably generated and maintained by the reorganization of the magnetic field of NOAA 11542. The reorganization of the magnetic-energy spectra occurs mainly for wave-numbers smaller than 0.2Mm-Mm-1 and the dissipation spectrum increases for wave-numbers around 1 Mm(-1).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Radio noise storms...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 29/10/2019 07:47 1.0 KiB 
4. Conditions of access and use
Languageen
Target Filesodre_raio.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/bibdigital/2013/09.29.20.43 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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7. Description control
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