Precise and effective fixed-pattern correction for logarithmic high dynamic range CMOS image sensors achieving low noise equivalent contrast over illumination

2012 ◽  
Author(s):  
M. Strobel
Keyword(s):  
Dynamic Range ◽  
High Dynamic Range ◽  
Low Noise ◽  
Image Sensors ◽  
Cmos Image Sensors ◽  
High Dynamic

A signal-to-noise ratio comparison of high dynamic range CMOS image sensors

2009 ◽  
Author(s):  
Leo H. C. Braga ◽  
Suzana Domingues ◽  
José G. Gomes ◽  
Antonio C. Mesquita
Keyword(s):  
Dynamic Range ◽  
Signal To Noise Ratio ◽  
High Dynamic Range ◽  
Image Sensors ◽  
Signal To Noise ◽  
Cmos Image Sensors ◽  
High Dynamic ◽  
Noise Ratio

A Charge Compensation Phototransistor for High-Dynamic-Range CMOS Image Sensors

2018 ◽  
Vol 65 (7) ◽  
pp. 2932-2938 ◽  
Author(s):  
Shuang Cui ◽  
Zhaohan Li ◽  
Chao Wang ◽  
Xiaotian Yang ◽  
Xinyang Wang ◽  
...  
Keyword(s):  
Dynamic Range ◽  
Charge Compensation ◽  
High Dynamic Range ◽  
Image Sensors ◽  
Cmos Image Sensors ◽  
High Dynamic ◽  
A Charge

scholarly journals A Tunable CMOS Image Sensor with High Fill-Factor for High Dynamic Range Applications

2020 ◽  
Vol 2 (1) ◽  
pp. 79
Author(s):  
Fernando de Souza Campos ◽  
Bruno Albuquerque de Castro ◽  
Jacobus W. Swart
Keyword(s):  
Bias Voltage ◽  
Fill Factor ◽  
Dynamic Range ◽  
Operation Mode ◽  
High Dynamic Range ◽  
Image Sensors ◽  
Control Voltage ◽  
Cmos Image Sensors ◽  
High Dynamic ◽  
High Fill Factor

Several CMOS imager sensors were proposed to obtain high dynamic range imager (>100 dB). However, as drawback these imagers implement a large number of transistors per pixel resulting in a low fill factor, high power consumption and high complexity CMOS image sensors. In this work, a new operation mode for 3 T CMOS image sensors is presented for high dynamic range (HDR) applications. The operation mode consists of biasing the conventional reset transistor as active load to photodiode generating a reference current. The output voltage achieves a steady state when the photocurrent becomes equal to the reference current, similar to the inverter operation in the transition region. At a specific bias voltage, the output swings from o to Vdd in a small light intensity range; however, high dynamic range is achieve using multiple readout at different bias voltage. For high dynamic range operation different values of bias voltage can be applied from each one, and the signal can be captured to compose a high dynamic range image. Compared to other high dynamic range architectures this proposed CMOS image pixel show as advantage high fill-factor (3 T) and lower complexity. Moreover, as the CMOS pixel does not operate in integration mode, de readout can be performed at higher speed. A prototype was fabricated at 3.3 V 0.35 µm CMOS technology. Experimental results are shown by applying five different control voltage from 0.65 to 1.2 V is possible to obtain a dynamic range of about 100 dB.

High-dynamic-range low-noise microwave amplifier

1970 ◽  
Vol 6 (7) ◽  
pp. 202
Author(s):  
J.R. Collard ◽  
A.R. Gobat
Keyword(s):  
Dynamic Range ◽  
High Dynamic Range ◽  
Low Noise ◽  
Microwave Amplifier ◽  
High Dynamic

scholarly journals High Dynamic Range Imaging at the Quantum Limit with Single Photon Avalanche Diode-Based Image Sensors

Sensors ◽  
2018 ◽  
Vol 18 (4) ◽  
pp. 1166 ◽  
Author(s):  
Neale Dutton ◽  
Tarek Al Abbas ◽  
Istvan Gyongy ◽  
Francescopaolo Mattioli Della Rocca ◽  
Robert Henderson
Keyword(s):  
Dynamic Range ◽  
Single Photon ◽  
High Dynamic Range ◽  
Image Sensors ◽  
Quantum Limit ◽  
High Dynamic Range Imaging ◽  
Range Imaging ◽  
Avalanche Diode ◽  
High Dynamic

scholarly journals Electronic Optical Sky Surveys

1998 ◽  
Vol 179 ◽  
pp. 49-55
Author(s):  
T.A. McKay
Keyword(s):  
Dynamic Range ◽  
Large Fraction ◽  
High Sensitivity ◽  
High Dynamic Range ◽  
Low Noise ◽  
Computer Hardware ◽  
Optical Detectors ◽  
Small Fields ◽  
Technical Advances ◽  
High Dynamic

The introduction of of Charge Coupled Devices (CCDs) in the middle 1970s provided astronomy with nearly perfect (linear, high-sensitivity, low-noise, high dynamic-range, digital) optical detectors. Unfortunately, restrictions imposed by CCD production and cost has typically limited their use to observations of relatively small fields. Recently a combination of technical advances have made practical the application of CCDs to survey science. CCD mosaic cameras, which help overcome the size restrictions imposed by CCD manufacture, allow electronic access to a larger fraction of the available focal plane. Multi-fiber spectrographs, which couple the low-noise, high QE performance of CCDs with the ability to observe spectra for many objects at once, have improved the spectroscopic efficiency of telescopes by factors approaching half a million. An improved understanding of image distortion gives us telescopes on which we expect sub-arcsecond images a large fraction of the time. Finally, and perhaps most important, the performance of computer hardware continues to advance, to the point where analysis of multi-terabyte datasets, while still daunting, is at least conceivable.

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