Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/Urn4h
Repositorysid.inpe.br/mtc-m17@80/2008/06.12.13.58   (restricted access)
Last Update2008:06.12.13.58.41 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2008/06.12.13.58.42
Metadata Last Update2018:06.05.03.30.50 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1007/s11207-008-9153-4
ISSN0038-0938
1573-093X
Citation KeyLaraBorgRosaDomi:2008:ShFlCo
TitleShort-Period Fluctuations in Coronal Mass Ejection Activity during Solar Cycle 23
Year2008
MonthMar.
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size388 KiB
2. Context
Author1 Lara, Alejandro
2 Borgazzi, Andrea
3 Rosa, Reinaldo Roberto
4 Domingues, Margarete Oliveira
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JJ5D
4 8JMKD3MGP5W/3C9JHQP
Group1
2 DGE-CEA-INPE-MCT-BR
3 LAC-CTE-INPE-MCT-BR
4 LAC-CTE-INPE-MCT-BR
Affiliation1 Instituto de Geofísica, Universidad Nacional Autónoma de México
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalSolar Physics
Volume248
Number1
Pages155-166
History (UTC)2008-06-12 13:58:42 :: simone -> administrator ::
2012-07-13 22:32:50 :: administrator -> simone :: 2008
2013-02-20 15:20:19 :: simone -> administrator :: 2008
2018-06-05 03:30:50 :: administrator -> marciana :: 2008
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsCME - Magnetic cycle - Solar activity
AbstractWe have constructed a time series of the number of coronal mass ejections (CMEs) observed by SOHO/LASCO during solar cycle 23. Using spectral analysis techniques (the maximum entropy method and wavelet analysis) we found short-period (< one year) semiperiodic activity. Among others, we found interesting periodicities at 193, 36, 28, and 25 days. We discuss the implications of such short-period activity in terms of the emergence and escape of magnetic flux from the convection zone, through the low solar atmosphere (where these periodicities have been found for numerous activity parameters), toward interplanetary space. This analysis shows that CMEs remove the magnetic flux in a quasiperiodic process in a way similar to that of magnetic flux emergence and other solar eruptive activity.
AreaCEA
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileshort period.pdf
User Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ESGTTP
8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
update 


Close