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dc.contributor.authorDe Jonghe, J.
dc.contributor.authorKuczyński, M. D.
dc.date.accessioned2024-02-28T15:30:06Z
dc.date.available2024-02-28T15:30:06Z
dc.date.issued2024-04
dc.identifier299619985
dc.identifier59425383-288b-4496-980b-ae626ab640e8
dc.identifier85182464024
dc.identifier.citationDe Jonghe , J & Kuczyński , M D 2024 , ' Neural network classification of eigenmodes in the magnetohydrodynamic spectroscopy code Legolas ' , Neural Computing and Applications , vol. 36 , pp. 5955–5964 . https://doi.org/10.1007/s00521-023-09403-1en
dc.identifier.issn1433-3058
dc.identifier.otherRIS: urn:8A1FACACD07FE3570CB0281E5160C79B
dc.identifier.otherRIS: De Jonghe2024
dc.identifier.otherORCID: /0000-0003-2443-3903/work/154531965
dc.identifier.urihttps://hdl.handle.net/10023/29371
dc.descriptionJDJ was supported by funding from the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme, Grant agreement No. 833251 PROMINENT ERC-ADG 2018.en
dc.description.abstractA neural network is employed to address a non-binary classification problem of plasma instabilities in astrophysical jets, calculated with the Legolas code. The trained models exhibit reliable performance in the identification of the two instability types supported by these jets. We also discuss the generation of artificial data and refinement of predictions in general eigenfunction classification problems.
dc.format.extent10
dc.format.extent1078464
dc.language.isoeng
dc.relation.ispartofNeural Computing and Applicationsen
dc.subjectMagnetohydrodynamicsen
dc.subjectEigenproblemen
dc.subjectNeural networken
dc.subjectSupervised learningen
dc.subjectClassificationen
dc.subjectDASen
dc.titleNeural network classification of eigenmodes in the magnetohydrodynamic spectroscopy code Legolasen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1007/s00521-023-09403-1
dc.description.statusPeer revieweden


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