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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3FCLLAL
Repositorysid.inpe.br/plutao/2013/12.12.18.39   (restricted access)
Last Update2014:01.16.16.20.00 (UTC) administrator
Metadata Repositorysid.inpe.br/plutao/2013/12.12.18.39.09
Metadata Last Update2018:06.04.23.39.25 (UTC) administrator
DOI10.1051/swsc/2013048
ISSN2115-7251
Labellattes: 3368023405805386 11 SaizCCDHNSBDDGMTV:2013:GeReSo
Citation KeySaizCCDHNSBDDGMTV:2013:GeReSo
TitleGeomagnetic response to solar and interplanetary disturbances
Year2013
Access Date2024, May 19
Secondary TypePRE PI
Number of Files1
Size2510 KiB
2. Context
Author 1 Saiz, Elena
 2 Cerrato, Yolanda
 3 Cid, Consuelo
 4 Dobrica, Venera
 5 Hejda, Pavel
 6 Nenovski, Petko
 7 Stauning, Peter
 8 Bochnicek, Josef
 9 Danov, Dimitar
10 Demetrescu, Crisan
11 Gonzalez, Walter Demetrio
12 Maris, Georgeta
13 Teodosiev, Dimitar
14 Valach, Fridich
Resume Identifier 1
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11 8JMKD3MGP5W/3C9JJC4
Group 1
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11 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation 1 Space Research Group-Space Weather, Departamento de Fı´sica, Universidad de Alcala´, Madrid, Spain
 2 Institute of Geodynamics, Romanian Academy, Bucharest, Romania
 3 Institute of Geophysics of the ASCR, Prague, Czech Republic
 4 National Institute for Geophysics, Geodesy and Geography, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria
 5 Institute for Space Research and Technologies, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria
 6 National Institute for Geophysics, Geodesy and Geography, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria
 7 Danish Meteorological Institute, Copenhagen, Denmark
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 9 Institute for Space Research and Technologies, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria
10 Institute of Geodynamics, Romanian Academy, Bucharest, Romania
11 Instituto Nacional de Pesquisas Espaciais (INPE)
12 Institute of Geodynamics, Romanian Academy, Bucharest, Romania
13 Institute for Space Research and Technologies, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria
14 Geomagnetic Observatory, Geophysical Institute, Slovak Academy of Sciences, Hurbanovo, Slovakia
Author e-Mail Address 1
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11 gonzalez@dge.inpe.br
e-Mail Addressgonzalez@dge.inpe.br
JournalJournal of Space Weather and Space Climate
Volume3
PagesA26
Secondary MarkB5
History (UTC)2013-12-12 18:39:09 :: lattes -> administrator ::
2018-06-04 23:39:25 :: administrator -> marcelo.pazos@inpe.br :: 2013
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordssolar activity
interplanetary medium
indices
ionosphere (general)
ring current
AbstractThe space weather discipline involves different physical scenarios, which are characterised by very different physical conditions, ranging from the Sun to the terrestrial magnetosphere and ionosphere. Thanks to the great modelling effort made during the last years, a few Sun-to-ionosphere/thermosphere physics-based numerical codes have been developed. However, the success of the prediction is still far from achieving the desirable results and much more progress is needed. Some aspects involved in this progress concern both the technical progress (developing and validating tools to forecast, selecting the optimal parameters as inputs for the tools, improving accuracy in prediction with short lead time, etc.) and the scientific development, i.e., deeper understanding of the energy transfer process from the solar wind to the coupled magnetosphere-ionosphere-thermosphere system. The purpose of this paper is to collect the most relevant results related to these topics obtained during the COST Action ES0803. In an end-to-end forecasting scheme that uses an artificial neural network, we show that the forecasting results improve when gathering certain parameters, such as X-ray solar flares, Type II and/or Type IV radio emission and solar energetic particles enhancements as inputs for the algorithm. Regarding the solar wind-magnetosphere-ionosphere interaction topic, the geomagnetic responses at high and low latitudes are considered separately. At low latitudes, we present new insights into temporal evolution of the ring current, as seen by Burtons equation, in both main and recovery phases of the storm. At high latitudes, the PCC index appears as an achievement in modelling the coupling between the upper atmosphere and the solar wind, with a great potential for forecasting purposes. We also address the important role of small-scale field-aligned currents in Joule heating of the ionosphere even under non-disturbed conditions. Our scientific results in the framework of the COST Action ES0803 cover the topics from the short-term solar-activity evolution, i.e., space weather, to the long-term evolution of relevant solar/heliospheric/magnetospheric parameters, i.e., space climate. On the timescales of the Hale and Gleissberg cycles (22- and 88-year cycle respectively) we can highlight that the trend of solar, heliospheric and geomagnetic parameters shows the solar origin of the widely discussed increase in geomagnetic activity in the last century.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Geomagnetic response to...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
User Grouplattes
marcelo.pazos@inpe.br
Reader Groupadministrator
marcelo.pazos@inpe.br
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.01.50 3
sid.inpe.br/bibdigital/2013/10.01.22.11 2
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsalternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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