Design requirements for high-sensitivity UV solar blind imaging detectors based on AlGaN/GaN photodetector arrays: a review

Computer Science

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Scientific paper

At present, band pass filtered, very high-gain photomultiplier tube (PMT) imaging sensors are employed to detect and image hot, UV emitting objects within the solar blind UV spectral region for wavelengths < 289 nm, either within or through the earth's atmosphere. In this paper we will reviews and summarize the stringent requirements that must be met in order to design AlGaN/GaN solar blind UV photodetector arrays that will have responsivities, detectivities, gain, speeds, and low noise levels comparable to those of present-day, high-gain PMT imaging detectors. Photodiode detectors operating in both the photovoltaic and photoconductive modes will be considered together with signal-gain that may be achieved through hybrid avalanche photodiodes and photodiodes operating in the pulsed Geiger mode.

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