Zn/Mg Co-Alloyed for Higher Photoelectric Performance and Unchanged Spectral Response in β-Ga2O3 Solar-Blind Photodetector

Author(s):  
Mengmeng Chang ◽  
Junhao Ye ◽  
Yuanli Su ◽  
Jingqin Shen ◽  
Nie Zhao ◽  
...  
2017 ◽  
Vol 13 (6) ◽  
pp. 483-488 ◽  
Author(s):  
Daoyou Guo ◽  
Xinyuan Qin ◽  
Ming Lv ◽  
Haoze Shi ◽  
Yuanli Su ◽  
...  

2021 ◽  
pp. 114645
Author(s):  
Zhisheng Lv ◽  
Lei Liu ◽  
Yan Sun ◽  
Xingyue Zhangyang ◽  
Feifei Lu ◽  
...  

2014 ◽  
Vol 22 (20) ◽  
pp. 24286 ◽  
Author(s):  
Guanghong Bao ◽  
Dabing Li ◽  
Xiaojuan Sun ◽  
Mingming Jiang ◽  
Zhiming Li ◽  
...  

Coatings ◽  
2021 ◽  
Vol 11 (10) ◽  
pp. 1178
Author(s):  
Min Zhang ◽  
Zhenjiang Li ◽  
Yunfei Zhao ◽  
Zhaofeng Wu ◽  
Jun Zhang ◽  
...  

In this study, ultraviolet detectors based on NaTaO3/TiO2 were fabricated with enhanced detection performance towards solar-blind (200–280 nm) light. A TiO2 seed layer was introduced and served as a buffer layer between the fluorine tin oxide (FTO)-coated glass substrate and the TiO2 film, which increased the adhesion between them. The periodic stability and photoelectric characteristics of the detectors were studied and analyzed. The detectors showed a high performance when illuminated by 265 nm and 254 nm UV light. At −15 V bias, the dark current of the detector was only 70 pA. Under the bias of −15 V and the illumination of 254 nm, the maximum photo-to-dark current ratio reached 20, and the response time was less than 300 ms. Moreover, the detector exhibited a fast response time and remained very stable after numerous testing cycles. These results demonstrate the potential application of NaTaO3/TiO2 composites in UV detection.


2021 ◽  
Vol 13 (37) ◽  
pp. 44509-44519
Author(s):  
Xuning Zhang ◽  
Xingyue Liu ◽  
Bo Sun ◽  
Haibo Ye ◽  
Chunhua He ◽  
...  

2014 ◽  
Vol 11 (3-4) ◽  
pp. 782-785
Author(s):  
L. E. Rodak ◽  
A. V. Sampath ◽  
C. S. Gallinat ◽  
J. Smith ◽  
Y. Chen ◽  
...  

2006 ◽  
Vol 37 (4) ◽  
pp. 336-339 ◽  
Author(s):  
C. Touzi ◽  
F. Omnès ◽  
T. Boufaden ◽  
P. Gibart ◽  
B. El Jani

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.


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