Publicación:
Onset-centered complexity signatures of GOES flare class in Konus-WIND G1–G3 time series

dc.contributor.authorSierra Porta, David
dc.contributor.authorPerez Navarro, Juan Diego
dc.contributor.authorPetro Ramos, Jesus David
dc.contributor.researchgroupGrupo de Investigación Gravitación y Matemática Aplicada
dc.contributor.seedbedsSemillero de Investigación en Astronomía y Ciencia de Datos
dc.date.accessioned2026-08-24T15:54:26Z
dc.date.issued2026-08-05
dc.descriptionContiene gráficos
dc.description.abstractThe high-energy emission from solar flares demonstrates highly variable and often complex light curves, whose temporal structure may contain information beyond standard amplitude-based summaries. Using the Konus-WIND solar flare observations, we carried out an investigation into the statistical association between the onset-centered changes in geometric and complexity-based descriptors and GOES flare classes. Our study was based on the data from the background-subtracted count rates from the event catalogue in three energy channels: G1 (20--80~keV), G2 (80--300~keV) and G3 (300--1200~keV). The observation of each event was segmented into pre-onset (``before'') and post-onset (``after'') intervals defined by bin boundaries relative to the trigger time. For each channel and segment we computed five descriptors: Higuchi fractal dimension, normalized permutation entropy, statistical complexity \(C_{JS}\) in the complexity--entropy framework, normalized Lempel--Ziv complexity (median-binarized), and Hjorth complexity. We summarized onset-associated changes by paired differences \(\Delta=\mathrm{after}-\mathrm{before}\) and assessed class dependence using nonparametric hypothesis tests with Benjamini--Hochberg false-discovery-rate control. In different channels, most descriptors showed non-zero onset-associated shifts, and the magnitude of \(\Delta\) was significantly different for most channel--descriptor combinations across GOES classes. The strongest monotonic class scaling was observed in the G1 channel for Higuchi fractal dimension, permutation entropy, and \(C_{JS}\), while the clearest separation in the G2 channel was provided by normalized Lempel--Ziv and Hjorth complexity, including a marked Hjorth-complexity transition for X-class events. In the G3 channel, onset-related changes remained evident but between-class discrimination was weaker overall, with Higuchi fractal dimension showing near class-invariant $\Delta$. The obtained results provide conservative population-level evidence that multi-channel onset-centered complexity and geometric descriptors are statistically related to flare class, and motivate future work on integrating additional physical covariates and strictly validated classification models.
dc.description.researchareaClima espacial y rayos cósmicos
dc.format.extent20 páginas
dc.format.mimetypeapplication/pdf
dc.identifier.citationD.Sierra-Porta, J. D.Pérez-Navarro,J. D. Petro-Ramos (2026). Onset-centered complexity signatures of GOES flare class in Konus-WIND G1–G3 time series. Advances in Space Research 78 (2026) pp. 7584-7599. doi:10.1016/j.asr.2026.07.121
dc.identifier.doi10.1016/j.asr.2026.07.121
dc.identifier.urihttps://hdl.handle.net/20.500.12585/14545
dc.language.isoeng
dc.publisherAdvances in Space Research
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dc.rights.licenseAtribución-NoComercial-SinDerivadas 4.0 Internacional (CC BY-NC-ND 4.0)
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subject.ddc520 - Astronomía y ciencias afines::523 - Cuerpos y fenómenos celestes específicos
dc.subject.lembSolar flares
dc.subject.lembSolar activity
dc.subject.lembSun -- Flares
dc.subject.lembSolar physics
dc.subject.lembSolar radiation
dc.subject.lembHigh -- energy astrophysics
dc.subject.lembFractal analysis
dc.subject.lembEntropy
dc.subject.lembTime-series analysis
dc.subject.lembStatistical methods
dc.subject.ocde1. Ciencias Naturales::1C. Ciencias físicas::1C08. Astronomía
dc.subject.ocde1. Ciencias Naturales::1A. Matemática::1A02. Matemáticas aplicadas
dc.subject.ocde1. Ciencias Naturales::1C. Ciencias físicas::1C05. Física de plasmas y fluidos
dc.subject.odsODS 17: Alianzas para lograr los objetivos. Fortalecer los medios de implementación y revitalizar la Alianza Mundial para el Desarrollo Sostenible
dc.subject.proposalSolar flares
dc.subject.proposalKonus-WIND
dc.subject.proposalGOES classification
dc.subject.proposalPermutation entropy
dc.subject.proposalStatistical complexity
dc.subject.proposalHiguchi fractal dimension
dc.subject.proposalHjorth parameters
dc.subject.proposalNonparametric tests
dc.subject.proposalFalse discovery rate
dc.titleOnset-centered complexity signatures of GOES flare class in Konus-WIND G1–G3 time series
dc.typeArtículo de revista
dc.type.coarhttp://purl.org/coar/resource_type/c_18cf
dc.type.coarversionhttp://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.contentDataPaper
dc.type.driverinfo:eu-repo/semantics/article
dc.type.redcolhttp://purl.org/redcol/resource_type/ART
dc.type.versioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication
relation.isAuthorOfPublication996a607a-3eb1-4484-8978-ed736b9fc0b7
relation.isAuthorOfPublicatione144acbd-d319-4f6e-8569-0e7e0a800d6e
relation.isAuthorOfPublication3a809cf6-b013-4aad-8e23-6dbad4c8d1b2
relation.isAuthorOfPublication.latestForDiscovery996a607a-3eb1-4484-8978-ed736b9fc0b7

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