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Representing Solar Active Regions with Triangulations

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dc.contributor.author Turmon, M. J. en_US
dc.contributor.author Mukhtar, S. en_US
dc.date.accessioned 2004-09-24T20:50:15Z
dc.date.available 2004-09-24T20:50:15Z
dc.date.issued 1998-08-23 en_US
dc.identifier.citation International Statistical Institute en_US
dc.identifier.citation Bristol, UK en_US
dc.identifier.clearanceno 98-0761 en_US
dc.identifier.uri http://hdl.handle.net/2014/19400
dc.description.abstract The solar chromosphere consists of three classes which contribute differently to ultraviolet radiation reaching the earth. We describe a data set of solar images, means of segmenting the images into the constituent classes, and novel high-level representation for compact objects based on a triangulation spatial 'membership function'. en_US
dc.format.extent 404368 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Triangulation chromosphere Markov chain Monte Carlo image segmentaion en_US
dc.title Representing Solar Active Regions with Triangulations en_US


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