dc.contributor.author | Riley, J. D. | en |
dc.contributor.author | Arridge, S. R. | en |
dc.contributor.author | Chrysanthou, Yiorgos L. | en |
dc.contributor.author | Dehghani, H. | en |
dc.contributor.author | Hillman, E. M. C. | en |
dc.contributor.author | Schweiger, M. | en |
dc.contributor.editor | Andersson-Engels S. | en |
dc.contributor.editor | Kaschke M.F. | en |
dc.creator | Riley, J. D. | en |
dc.creator | Arridge, S. R. | en |
dc.creator | Chrysanthou, Yiorgos L. | en |
dc.creator | Dehghani, H. | en |
dc.creator | Hillman, E. M. C. | en |
dc.creator | Schweiger, M. | en |
dc.date.accessioned | 2019-11-13T10:42:06Z | |
dc.date.available | 2019-11-13T10:42:06Z | |
dc.date.issued | 2001 | |
dc.identifier.uri | http://gnosis.library.ucy.ac.cy/handle/7/54897 | |
dc.description.abstract | We present the Radiosity-Diffusion model in three dimensions (3D), as an extension to previous work in 2D. It is a method for handling non-scattering spaces in optically participating media. We present the extension of the model to 3D including an extension to the model to cope with increased complexity of the 3D domain. We show that in 3D more careful consideration must be given to the issues of meshing and visibility to model the transport of light within reasonable computational bounds. We demonstrate the model to be comparable to Monte-Carlo simulations for selected geometries, and show preliminary results of comparisons to measured time-resolved data acquired on resin phantoms. | en |
dc.source | Proceedings of SPIE - The International Society for Optical Engineering | en |
dc.source | Photon Migration, Optical Coherence Tomography, and Microscopy | en |
dc.source.uri | https://www.scopus.com/inward/record.uri?eid=2-s2.0-0035760913&doi=10.1117%2f12.447415&partnerID=40&md5=89510a8c65930d17d78dda12ea81efb2 | |
dc.subject | Mathematical models | en |
dc.subject | Computer simulation | en |
dc.subject | Monte Carlo methods | en |
dc.subject | Tomography | en |
dc.subject | Diffusion | en |
dc.subject | Light transmission | en |
dc.subject | Light Propagation | en |
dc.subject | Non-Scattering | en |
dc.subject | Optical Tomography | en |
dc.subject | Participating Media | en |
dc.subject | Radiosity | en |
dc.subject | Transport Equation | en |
dc.subject | Voids | en |
dc.title | The Radiosity Diffusion model in 3D | en |
dc.type | info:eu-repo/semantics/conferenceObject | |
dc.identifier.doi | 10.1117/12.447415 | |
dc.description.volume | 4431 | |
dc.description.startingpage | 153 | |
dc.description.endingpage | 164 | |
dc.author.faculty | 002 Σχολή Θετικών και Εφαρμοσμένων Επιστημών / Faculty of Pure and Applied Sciences | |
dc.author.department | Τμήμα Πληροφορικής / Department of Computer Science | |
dc.type.uhtype | Conference Object | en |
dc.description.notes | <p>Sponsors: OSA | en |
dc.description.notes | SPIE | en |
dc.description.notes | Conference code: 59923 | en |
dc.description.notes | Cited By :6</p> | en |
dc.contributor.orcid | Chrysanthou, Yiorgos L. [0000-0001-5136-8890] | |
dc.gnosis.orcid | 0000-0001-5136-8890 | |