Publicación: Onset-centered complexity signatures of GOES flare class in Konus-WIND G1–G3 time series
| dc.contributor.author | Sierra Porta, David | |
| dc.contributor.author | Perez Navarro, Juan Diego | |
| dc.contributor.author | Petro Ramos, Jesus David | |
| dc.contributor.researchgroup | Grupo de Investigación Gravitación y Matemática Aplicada | |
| dc.contributor.seedbeds | Semillero de Investigación en Astronomía y Ciencia de Datos | |
| dc.date.accessioned | 2026-08-24T15:54:26Z | |
| dc.date.issued | 2026-08-05 | |
| dc.description | Contiene gráficos | |
| dc.description.abstract | The 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.researcharea | Clima espacial y rayos cósmicos | |
| dc.format.extent | 20 páginas | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | D.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.doi | 10.1016/j.asr.2026.07.121 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12585/14545 | |
| dc.language.iso | eng | |
| dc.publisher | Advances in Space Research | |
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| dc.rights.license | Atribución-NoComercial-SinDerivadas 4.0 Internacional (CC BY-NC-ND 4.0) | |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | |
| dc.subject.ddc | 520 - Astronomía y ciencias afines::523 - Cuerpos y fenómenos celestes específicos | |
| dc.subject.lemb | Solar flares | |
| dc.subject.lemb | Solar activity | |
| dc.subject.lemb | Sun -- Flares | |
| dc.subject.lemb | Solar physics | |
| dc.subject.lemb | Solar radiation | |
| dc.subject.lemb | High -- energy astrophysics | |
| dc.subject.lemb | Fractal analysis | |
| dc.subject.lemb | Entropy | |
| dc.subject.lemb | Time-series analysis | |
| dc.subject.lemb | Statistical methods | |
| dc.subject.ocde | 1. Ciencias Naturales::1C. Ciencias físicas::1C08. Astronomía | |
| dc.subject.ocde | 1. Ciencias Naturales::1A. Matemática::1A02. Matemáticas aplicadas | |
| dc.subject.ocde | 1. Ciencias Naturales::1C. Ciencias físicas::1C05. Física de plasmas y fluidos | |
| dc.subject.ods | ODS 17: Alianzas para lograr los objetivos. Fortalecer los medios de implementación y revitalizar la Alianza Mundial para el Desarrollo Sostenible | |
| dc.subject.proposal | Solar flares | |
| dc.subject.proposal | Konus-WIND | |
| dc.subject.proposal | GOES classification | |
| dc.subject.proposal | Permutation entropy | |
| dc.subject.proposal | Statistical complexity | |
| dc.subject.proposal | Higuchi fractal dimension | |
| dc.subject.proposal | Hjorth parameters | |
| dc.subject.proposal | Nonparametric tests | |
| dc.subject.proposal | False discovery rate | |
| dc.title | Onset-centered complexity signatures of GOES flare class in Konus-WIND G1–G3 time series | |
| dc.type | Artículo de revista | |
| dc.type.coar | http://purl.org/coar/resource_type/c_18cf | |
| dc.type.coarversion | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |
| dc.type.content | DataPaper | |
| dc.type.driver | info:eu-repo/semantics/article | |
| dc.type.redcol | http://purl.org/redcol/resource_type/ART | |
| dc.type.version | info:eu-repo/semantics/publishedVersion | |
| dspace.entity.type | Publication | |
| relation.isAuthorOfPublication | 996a607a-3eb1-4484-8978-ed736b9fc0b7 | |
| relation.isAuthorOfPublication | e144acbd-d319-4f6e-8569-0e7e0a800d6e | |
| relation.isAuthorOfPublication | 3a809cf6-b013-4aad-8e23-6dbad4c8d1b2 | |
| relation.isAuthorOfPublication.latestForDiscovery | 996a607a-3eb1-4484-8978-ed736b9fc0b7 |
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