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dc.contributor.authorZakovic, S.
dc.contributor.authorUlanowski, Zbigniew
dc.contributor.authorBartholomew-Biggs, Michael
dc.date.accessioned2011-11-08T12:01:14Z
dc.date.available2011-11-08T12:01:14Z
dc.date.issued1998
dc.identifier.citationZakovic , S , Ulanowski , Z & Bartholomew-Biggs , M 1998 , ' Application of global optimisation to particle identification using light scattering ' , Inverse Problems , vol. 14 , no. 4 , pp. 1053-1067 . https://doi.org/10.1088/0266-5611/14/4/019
dc.identifier.issn0266-5611
dc.identifier.otherPURE: 445006
dc.identifier.otherPURE UUID: fb91e795-6ed2-499a-b3c6-67027ad57564
dc.identifier.otherScopus: 0000365207
dc.identifier.otherORCID: /0000-0003-4761-6980/work/32374682
dc.identifier.urihttp://hdl.handle.net/2299/6935
dc.description‘In these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.’ Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical Society
dc.description.abstractNumerical methods of solving the inverse light scattering problem for spheres are presented. The methods are based on two stochastic global optimization techniques: Deep's random search and the multilevel single-linkage clustering analysis due to Rinnooy Kan and Timmer. Computational examples show that the radius and the refractive index of spheres comparable with or larger than the wavelength of light can be recovered from multiangle scattering data. While the random search approach is faster, the clustering analysis is shown to be more reliable. A general discussion of the clustering method is also given.en
dc.format.extent15
dc.language.isoeng
dc.relation.ispartofInverse Problems
dc.titleApplication of global optimisation to particle identification using light scatteringen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1088/0266-5611/14/4/019
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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