1999
DOI: 10.1117/12.344560
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Solar-blind UV region and UV detector development objectives

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Cited by 81 publications
(29 citation statements)
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“…These promising properties have inspired the use of III-nitride semiconductors for many applications such as light-emitting diodes, laser diodes, photodetectors, high electron mobility transistors, field-effect transistors, Schottky diodes, and solar cells [1][2][3][4][5]. Among these applications, ultraviolet (UV) photodetectors that are usable in visible-to solar-blind conditions have drawn significant attention for use in missile plume detection, flame engine sensors, ozone layer monitoring, and secure intersatellite communication systems [6,7]. With a bandgap between those of GaN (3.4 eV) and AlN (6.2 eV) [8], AlGaN can be used in both visible-and solar-blind UV photodetectors without bulky filter systems or heavy cooling systems such as those required for Si-based photodetectors, thus reducing the footprint and the production cost of the devices [7].…”
Section: Introductionmentioning
confidence: 99%
“…These promising properties have inspired the use of III-nitride semiconductors for many applications such as light-emitting diodes, laser diodes, photodetectors, high electron mobility transistors, field-effect transistors, Schottky diodes, and solar cells [1][2][3][4][5]. Among these applications, ultraviolet (UV) photodetectors that are usable in visible-to solar-blind conditions have drawn significant attention for use in missile plume detection, flame engine sensors, ozone layer monitoring, and secure intersatellite communication systems [6,7]. With a bandgap between those of GaN (3.4 eV) and AlN (6.2 eV) [8], AlGaN can be used in both visible-and solar-blind UV photodetectors without bulky filter systems or heavy cooling systems such as those required for Si-based photodetectors, thus reducing the footprint and the production cost of the devices [7].…”
Section: Introductionmentioning
confidence: 99%
“…Ultraviolet radiated by corona is also used to detect corona. Because of the solar blind band exists, UV in 220-280nm is rectangular distribution in atmosphere 4,5,6,7 . The lights from corona have this kind of UV light.…”
Section: Corona Detection Methodsmentioning
confidence: 99%
“…For solar-blind UV absorption the cut-off wavelength should be below 280 nm (4.5 eV) [1][2][3] corresponding to a significantly larger bandgap than that of ZnO (3.37 eV). Alloying ZnO with MgO, which is reasonably traditional, leads to the ternary compound MgZnO [4,5] with tunable bandgap up to 4.55 eV in wurtzite phase [6].…”
Section: Introductionmentioning
confidence: 99%