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dc.contributor.authorScully, Jeremiah
dc.contributor.authorFlynn, Ronan
dc.contributor.authorGallagher, Peter T.
dc.contributor.authorCarley, Eoghan P.
dc.contributor.authorDaly, Mark
dc.date.accessioned2024-04-29T12:19:20Z
dc.date.available2024-04-29T12:19:20Z
dc.date.copyright2023
dc.date.issued2023-06
dc.identifier.citationSculy, J., Flynn, R., Gallagher, P.T., Carley, E.P., Daly, M. (2023). Improved type III solar radio bust detection using congruent deep learning models. Astronomy & Astrophysics. 674, A218. doi.org/10.1051/0004-6361/202346404en_US
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://research.thea.ie/handle/20.500.12065/4811
dc.description.abstractSolar flares are energetic events in the solar atmosphere that are often linked with solar radio bursts (SRBs). SRBs are observed at metric to decametric wavelengths and are classified into five spectral classes (Type I–V) based on their signature in dynamic spectra. The automatic detection and classification of SRBs is a challenge due to their heterogeneous form. Near-real time detection and classification of SRBs has become a necessity in recent years due to large data rates generated by advanced radio telescopes such as the LOw Frequency ARray (LOFAR). For this study, we implemented congruent deep learning models to automatically detect and classify Type III SRBs. We generated simulated Type III SRBs, which were comparable to Type IIIs seen in real observations, using a deep learning method known as the generative adversarial network (GAN). This simulated data were combined with observations from LOFAR to produce a training set that was used to train an object detection model known as you only look once (YOLOv2). Using this congruent deep learning model system, we can accurately detect Type III SRBs at a mean Average Precision (mAP) value of 77.71%en_US
dc.formatPDFen_US
dc.language.isoengen_US
dc.rightsAttribution 4.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/us/*
dc.subjectSun: heliosphereen_US
dc.subjectSun: particle emissionen_US
dc.subjectSun: flaresen_US
dc.titleImproved type III solar radio bust detection using congruent deep learning modelsen_US
dc.typeinfo:eu-repo/semantics/articleen_US
dc.contributor.affiliationTechnological University of the Shannon: Midlands Midwesten_US
dc.contributor.sponsorScience Foundation Ireland (SFI), Department of Business, Enterprise and Innovation, Open Eir and O aly County Council. J. Scully acknowledges support from SFI and the Technological University of the Shannon (TUS).en_US
dc.description.peerreviewyesen_US
dc.identifier.doi10.1051/0004-6361/202346404en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6475-005Xen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6475-005Xen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6106-5292en_US
dc.identifier.volume674en_US
dc.rights.accessrightsinfo:eu-repo/semantics/openAccessen_US
dc.subject.departmentDepartment of Computer and Software Engineering: TUS Midlandsen_US
dc.type.versioninfo:eu-repo/semantics/publishedVersionen_US


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Attribution 4.0 United States
Except where otherwise noted, this item's license is described as Attribution 4.0 United States