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dc.contributor.authorDamé, L.
dc.contributor.authorGhorbel, H.
dc.contributor.authorMeftah, M.
dc.contributor.authorArrateig, X.
dc.contributor.authorGilbert, P.
dc.contributor.authorMaso, P.
dc.contributor.authorBolsée, D.
dc.contributor.authorPereira, N.
dc.contributor.authorRogers, D.
dc.contributor.authorBove, P.
dc.contributor.authorSandana, V.
dc.contributor.authorTeherani, F.
dc.date2022
dc.date.accessioned2022-03-29T08:07:52Z
dc.date.available2022-03-29T08:07:52Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/9890
dc.descriptionWe present measurement protocols of performances, test and calibrations of new compact solid-state photodetectors based on β-Ga2O3 oxides, and optimized for the UVC. They present reduced dark currents, permitting room temperature operation suppressing need for a cooling system (mass and power savings) and avoiding cold surfaces that traps environmental contamination. Detectors' response peak around 215-220 nm with a bandpass of 30 nm, allowing to observe the UVC wavelength band responsible of ozone creation in the stratosphere (Herzberg continuum, 200-242 nm) and to achieve solar-blindness for wavelengths above 250 nm. Other key assets of β-Ga2O3 detectors are their radiation hard properties (longer lifetime), and possible sensitivity (several hundreds mA/W at -5 V) that allows operation at lower voltages (reduced power), a key asset for Space applications. These detectors, evaluated, tested and calibrated, will be integrated on the INSPIRE-7 nanosatellite to be launched in 2023.
dc.languageeng
dc.titlePerformances and calibrations of new disruptive UVC β-Ga2O3 sensors for new space applications
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeOzone
dc.subject.freeSpace sensors
dc.subject.freeOxides
dc.subject.freePhotodetectors
dc.subject.freeStratosphere
dc.subject.freeVisible radiation
dc.source.titleProceedings of SPIE PC12002 - Oxide-based Materials and Devices XIII
dc.source.volumePC12002
dc.source.pagePC120020F
Orfeo.peerreviewedNo
dc.identifier.doi10.1117/12.2610749
dc.identifier.scopus


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