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dc.contributor.authorFarup, Ivar
dc.date.accessioned2014-07-22T07:08:04Z
dc.date.available2014-07-22T07:08:04Z
dc.date.issued2014
dc.identifier.citationFarup, I. (2014) Hyperbolic geometry for colour metrics. In: Optics Express, 22(10), p. 12369-12378.nb_NO
dc.identifier.issn1094-4087
dc.identifier.urihttp://hdl.handle.net/11250/197892
dc.descriptionThis is an Open Access article. This paper was published in Optics Express and is made available as an electronic reprint with the permission of OSA. The paper can be found at the following URL on the OSA website: http://dx.doi.org/10.1364/OE.22.012369. Systematic or multiple reproduction or distribution to multiple locations via electronic or other means is prohibited and is subject to penalties under law.nb_NO
dc.description.abstractIt is well established from both colour difference and colour order perpectives that the colour space cannot be Euclidean. In spite of this, most colour spaces still in use today are Euclidean, and the best Euclidean colour metrics are performing comparably to state-of-the-art non-Euclidean metrics. In this paper, it is shown that a transformation from Euclidean to hyperbolic geometry (i.e., constant negative curvature) for the chromatic plane can significantly improve the performance of Euclidean colour metrics to the point where they are statistically significantly better than state-of-the-art non-Euclidean metrics on standard data sets. The resulting hyperbolic geometry nicely models both qualitatively and quantitatively the hue super-importance phenomenon observed in colour order systems.nb_NO
dc.language.isoengnb_NO
dc.publisherThe Optical Societynb_NO
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Informasjons- og kommunikasjonsvitenskap: 420::Simulering, visualisering, signalbehandling, bildeanalyse: 429nb_NO
dc.titleHyperbolic geometry for colour metricsnb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.source.pagenumber12369-12378nb_NO
dc.source.volume22nb_NO
dc.source.journalOptics Expressnb_NO
dc.source.issue10nb_NO


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