Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3P8SECKy/EpUcH
Repositorysid.inpe.br/jeferson/2004/12.09.14.22   (restricted access)
Last Update2006:06.14.04.17.00 (UTC) administrator
Metadata Repositorysid.inpe.br/jeferson/2004/12.09.14.22.57
Metadata Last Update2021:07.18.04.01.46 (UTC) administrator
Secondary KeyINPE-10988-PRE/6444
ISSN1364-6826
Citation KeyEcherGGPVDGS:2004:LoTeCo
TitleLong term correlation between solar and geomagnetic activity
Year2004
MonthMar.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size285 KiB
2. Context
Author1 Echer, Ezequiel
2 Gonzalez, Walter Demetrio
3 Gonzalez, Alicia Luisa Clua de
4 Prestes, A.
5 Vieira, Luis Eduardo A.
6 Dal Lago, Alisson
7 Guarnieri, Fernando Luis
8 Schuch, Nelson Jorge
Resume Identifier1 8JMKD3MGP5W/3C9JH3D
2 8JMKD3MGP5W/3C9JJC4
3
4
5
6 8JMKD3MGP5W/3C9JGH3
7
8 8JMKD3MGP5W/3C9JHUD
Group1 DGE-INPE-MCT-BR
2 RSU-INPE-MCT-BR
3
4
5
6
7
8
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume66
Number12
Pages1019-1025
History (UTC)2004-12-09 16:22:58 :: alexandra -> marciana ::
2006-06-06 14:40:25 :: marciana -> administrator ::
2007-03-09 22:30:03 :: administrator -> marciana ::
2008-05-02 16:20:27 :: marciana -> administrator ::
2021-07-18 04:01:46 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGeomagnetic activity
Solar activity
Solar wind
Sunspot number
AbstractA long-term correlation study between solar and geomagnetic activity is reported in this work using annual averages of the aa index and of the sunspot number Rz in the period of 1868?2000. Dst and AE geomagnetic indices and solar wind speed data are used for more recent periods. It is shown that the geomagnetic and solar activity correlation has decreased since the end of the 19th century, and the lag between them has increased. The variations of Rz and aa were in phase in the early period (solar cycles 11?14, around 1868?1910), and became out of phase in later periods (with a lag of 2 years in solar cycle 22, with aa maximum after Rz). Nevertheless, this trend is not monotonic and superposed <uctuations are seen, which does not permit determine if this correlation decrease is part or not of a long period solar activity cycle. The probable cause of the correlation decrease seems to be related to the aa index dual peak structure. The second aa peak seems to have increased relative to the =rst one. This second peak is more related to the high-speed streams originated from co-rotating structures whereas the =rst one is related to sunspot (coronal mass ejections) activity. In recent periods, since 1964, it has been observed that aa annual values have higher correlation with the fraction of days per year with daily solar wind speed peaks larger than 500 km=s (Fpk) than with Rz . The aa index also shows larger correlation with AE index than with Dst. Thus, it seems that average aa is strongly in<uenced by AE activity, which is in<uenced mainly by high speed streams from coronal holes. One can conclude that the decrease in correlation between aa and Rz occurs because the second aa peak has becoming stronger relative to the =rst one. The cause seems to be that open solar magnetic =eld structures have increased their activity relative to the closed (sunspot-related) solar magnetic =eld structures. This implies that the global solar magnetic =eld could have experienced a di?erential (between closed and open structures) large-scale variation in the last 130 years. c 2004 Elsevier Ltd. All rights reserved.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Long term correlation...
Arrangement 2urlib.net > CRCRS > Long term correlation...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filesdarticle.pdf
User Groupadministrator
alexandra
marciana
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsaffiliation alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi 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