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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3HG7EFL
Repositorysid.inpe.br/plutao/2014/12.01.12.30   (restricted access)
Last Update2014:12.09.12.38.15 (UTC) administrator
Metadata Repositorysid.inpe.br/plutao/2014/12.01.12.30.04
Metadata Last Update2021:07.28.22.09.15 (UTC) administrator
DOI10.1016/j.knosys.2014.07.012
ISSN0950-7051
1872-7409
Labellattes: 6513046926936437 3 PoliLlCeSaPeRaNi:2014:SoFlDe
Citation KeyPoliLlCeSaPeRaNi:2014:SoFlDe
TitleSolar flare detection system based on tolerance near sets in a GPU-CUDA framework
Year2014
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI {} 0950-7051 {PRE PI}
Number of Files1
Size4364 KiB
2. Context
Author1 Poli, G.
2 Llapa, E.
3 Cecatto, José Roberto
4 Saito, J. H.
5 Peters, J. F.
6 Ramanna, S.
7 Nicoletti, M. C.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHJB
Group1
2
3 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1
2
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4
5 james.peters3@ad.umanitoba.ca
e-Mail Addressmarcelo.pazos@inpe.br
JournalKnowledge Based Systems
Volume70
Pages345-360
Secondary MarkA2_ENGENHARIAS_IV B1_CIÊNCIA_DA_COMPUTAÇÃO B1_INTERDISCIPLINAR
History (UTC)2014-12-01 12:30:04 :: lattes -> administrator ::
2021-07-28 22:09:15 :: administrator -> marcelo.pazos@inpe.br :: 2014
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsTolerance near sets
Flare detection
Pattern recognition
GPU-CUDA
AbstractThis article presents a unique application of tolerance near sets (TNS) for detecting solar flare events in solar images acquired using radio astronomy techniques. In radio astronomy (RA) applications, the interferometric array processing of data streams presents algorithmic and response time challenges as well as a high volume of data. The radio interferometer is an RA instrument composed of an array of antennas. Radio signals emitted by a celestial object are captured by the antennas and are subsequently processed in such a way that each pair of antennas produces correlated data. The overall correlated data is then accumulated and, after an integration period, the spectral image of the observed object is obtained. The process of deconvolution of the spectral image produces the desired spatial image of the celestial object. The proposed solar flare detection system is embedded in a computational platform framework suitable for dealing with huge volumes of data, based on a cluster of CPUGPU pairs. The experimental results presented in the paper include comparison of the TNS-based algorithm (implemented as the SOL-FLARE system) with the K-means algorithm using significant samples of test images to validate the detection system. The performances of both systems are comparatively analyzed using Receiver Operating Characteristic (ROC) curves. The images used in the experiments were selected from a data repository produced by the Nobeyama Radioheliograph, in Japan, during the years 2004 up to 2013. The main contribution of the article is a novel approach to solar flare detection in a GPUCUDA framework.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Solar flare detection...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1-s2.0-S095070511400269X-main.pdf
User Grouplattes
marcelo.pazos@inpe.br
Reader Groupadministrator
marcelo.pazos@inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
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/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.52.30 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
NotesSetores de Atividade: Pesquisa e desenvolvimento científico.
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition number orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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