dc.contributor.author | Scully, Jeremiah | |
dc.contributor.author | Flynn, Ronan | |
dc.contributor.author | Gallagher, Peter T. | |
dc.contributor.author | Carley, Eoghan P. | |
dc.contributor.author | Daly, Mark | |
dc.date.accessioned | 2024-04-29T12:19:20Z | |
dc.date.available | 2024-04-29T12:19:20Z | |
dc.date.copyright | 2023 | |
dc.date.issued | 2023-06 | |
dc.identifier.citation | Sculy, 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/10.1051/0004-6361/202346404 | en_US |
dc.identifier.issn | 0004-6361 | |
dc.identifier.issn | 1432-0746 | |
dc.identifier.uri | https://research.thea.ie/handle/20.500.12065/4811 | |
dc.description.abstract | Solar 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.format | PDF | en_US |
dc.language.iso | eng | en_US |
dc.rights | Attribution 4.0 United States | * |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/us/ | * |
dc.subject | Sun: heliosphere | en_US |
dc.subject | Sun: particle emission | en_US |
dc.subject | Sun: flares | en_US |
dc.title | Improved type III solar radio bust detection using congruent deep learning models | en_US |
dc.type | info:eu-repo/semantics/article | en_US |
dc.contributor.affiliation | Technological University of the Shannon: Midlands Midwest | en_US |
dc.contributor.sponsor | Science 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.peerreview | yes | en_US |
dc.identifier.doi | 10.1051/0004-6361/202346404 | en_US |
dc.identifier.orcid | https://orcid.org/0000-0002-6475-005X | en_US |
dc.identifier.orcid | https://orcid.org/0000-0002-6475-005X | en_US |
dc.identifier.orcid | https://orcid.org/0000-0002-6106-5292 | en_US |
dc.identifier.volume | 674 | en_US |
dc.rights.accessrights | info:eu-repo/semantics/openAccess | en_US |
dc.subject.department | Department of Computer and Software Engineering: TUS Midlands | en_US |
dc.type.version | info:eu-repo/semantics/publishedVersion | en_US |