Representing Solar Active Regions with Triangulations

Turmon, M. J.; Mukhtar, S.

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