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dc.contributor.authorPeyaud, A
dc.contributor.authorAngelopoulos, A
dc.contributor.authorChelmis, C
dc.contributor.authorCostopoulos, V
dc.contributor.authorChica Serrano, Manuel 
dc.contributor.authorGiomataris, I
dc.contributor.authorGongadze, A
dc.contributor.authorHerbert, T
dc.contributor.authorKantemiris, I
dc.contributor.authorKirch, S
dc.contributor.authorMols, J
dc.contributor.authorPapaevangelou, T
dc.contributor.authorPavlopoulos, P
dc.contributor.authorQuinlan, F
dc.date.accessioned2024-11-22T07:30:19Z
dc.date.available2024-11-22T07:30:19Z
dc.date.issued2015
dc.identifier.citationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 787 102-104es_ES
dc.identifier.urihttps://hdl.handle.net/10481/97233
dc.description.abstractThe objective of the ForFire project is the development of an outdoor fire detection system by using an innovative solar blind camera based on the technology of photosensitive gas and solid-state detectors. The development of this new sensor together with an appropriate algorithm for pattern recognition aims to provide a high capability and a high reliability flame-detection system with cost effectiveness, early detection and accurate localization of fire hazards. This is achieved by focusing specifically on the detection of the VUV part (180 nmrλr260 nm) of the electromagnetic spectrum emitted by the fire source. The advantage of this approach is that on Earth only fire flames emit in this spectral range thus avoiding potential interferences with other wavelength sources where the Sun is a dominant background.es_ES
dc.language.isoenges_ES
dc.titleForfire photodetectores_ES
dc.typejournal articlees_ES
dc.relation.projectIDFP7 Forfire (FP7-SME-2008-1)es_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doihttps://doi.org/10.1016/j.nima.2014.11.044


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