• 센서학회지
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• 제25권5호
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• pp.349-353
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• 2016

Recently, research on bolometer-type uncooled infrared image sensor which is made for industrial applications has been increasing. In general, it is difficult to calibrate fixed pattern noise (FPN) of bolometer array. In this paper, average-current calibration algorithm is presented for reducing bolometer resistance offset. A resistor which is produced by standard CMOS process, on the average, has a deviation. We compensate for deviation of each resistor using average-current calibration algorithm. The proposed algorithm has been implemented by a chip which is consisted of a bolometer pixel array, average current generators, current-to-voltage converters (IVCs), a digital-to-analog converter (DAC), and analog-to-digital converters (ADCs). These bolometer-resistor array and readout circuit were designed and manufactured by $0.35{\mu}m$ standard CMOS process.

• 전기학회논문지
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• 제60권2호
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• pp.320-324
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• 2011

A digital technique is adopted to calibrate the current mismatch of the charge pump (CP) in phase-locked loops. A 2 GHz charge pump PLL (CPPLL) is used to justify the proposed calibration technique. The proposed digital calibration technique is implemented simply using a counter. The proposed calibration technique reduces the calibration time by up to a maximum of 50% compared other with techniques. Also by using a dual-mode CP, good current matching characteristics can be achieved to compensate $0.5{\mu}A$ current mismatch in CP. It was designed in a standard $0.13{\mu}m$ CMOS technology. The maximum calibration time is $33.6{\mu}s$ and the average power is 18.38mW with 1.5V power supply and effective area is $0.1804mm^2$.

• 한국태양에너지학회:학술대회논문집
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• 한국태양에너지학회 2012년도 춘계학술발표대회 논문집
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• pp.182-187
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• 2012

Since PV PCS uses output current sensor for ac output current control, the sensor's sensing value includes unnecessary offset inevitably. If PV inverter is controlled by the included offset value, it's output current will generate DC offset. The DC offset of output current for trans-less PV inverter is fatal to grid, which results in saturating grid side transformer. Usually DSP controller of PV inverter reads several times sensing value during initial operation and, finally, it's average value is used for offset calibration. However, if temperature changes, the offset changes, too. Therefore, output current sensor measures sensing value that includes offset again. In this paper we propose new algorithm where two identical forward and reverse sensors are used to calculate the offset in real time. As a result the offset is not correlated with temperature change. The proposed algorithm is verified through PSIM simulation for validity.

• Journal of Information Processing Systems
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• 제15권5호
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• pp.1082-1095
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• 2019

Camera calibration is an important part of machine vision and close-range photogrammetry. Since current calibration methods fail to obtain ideal internal and external camera parameters with limited computing resources on mobile terminals efficiently, this paper proposes an improved fast camera calibration method for mobile terminals. Based on traditional camera calibration method, the new method introduces two-order radial distortion and tangential distortion models to establish the camera model with nonlinear distortion items. Meanwhile, the nonlinear least square L-M algorithm is used to optimize parameters iteration, the new method can quickly obtain high-precise internal and external camera parameters. The experimental results show that the new method improves the efficiency and precision of camera calibration. Terminals simulation experiment on PC indicates that the time consuming of parameter iteration reduced from 0.220 seconds to 0.063 seconds (0.234 seconds on mobile terminals) and the average reprojection error reduced from 0.25 pixel to 0.15 pixel. Therefore, the new method is an ideal mobile terminals camera calibration method which can expand the application range of 3D reconstruction and close-range photogrammetry technology on mobile terminals.

• 한국태양에너지학회 논문집
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• 제32권spc3호
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• pp.255-261
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• 2012

Since PV PCS uses output current sensor for ac output current control, the sensor's sensing value includes unnecessary offset inevitably. If PV inverter is controlled by the included offset value, it's output current will generate DC offset. The DC offset of output current for trans-less PV inverter is fatal to grid, which results in saturating grid side transformer. Usually DSP controller of PV inverter reads several times sensing value during initial operation and, finally, it's average value is used for offset calibration. However, if temperature changes, the offset changes, too. And also, the switch device is not ideal, both each switching element of the voltage drop difference and on & off time delay difference generate DC offset. Thus, to compensate for deadtime and the switch voltage drop, feedback control by output current DC offset should be provided to compensate additional distortion of the output current. The validity of the proposed method is confirmed through PSIM simulation.

• 한국전자파학회논문지
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• 제29권7호
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• pp.484-490
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• 2018

본 논문은 13.56 MHz 임피던스 자동 정합 시스템 내의 VI 센서를 이용하여 전압 신호와 전류 신호를 측정하고, 부하임피던스를 계산하는 새로운 알고리즘에 대해서 기술하였다. 기존의 $50{\Omega}$ 교정 부하로 하던 방식에서 벗어나 임의의 복소수 교정 부하를 사용하여 에러율이 향상되는 알고리즘을 제안한다. 에러율은 $R_{IN}$ 평균 1 % 이하, $X_{IN}$은 평균 20 %이하 목표로 한다. 일차적으로 믹서를 사용하여 IF 주파수를 계산하여 에러율을 줄였고, 두 번째로 임의의 복소수 부하를 교정 부하로 사용하였을 때 에러율이 $R_{IN}$은 평균 2.7 %에서 평균 0.3 %로 감소하였고, $X_{IN}$은 평균 102 %에서 평균 18.3%까지 감소하였습니다.

• Current Optics and Photonics
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• 제5권5호
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• pp.524-531
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• 2021

In an integral-imaging microscopy (IIM) system, a microlens array (MLA) is the primary optical element; however, surface errors impede the resolution of a raw image's details. Calibration is a major concern with regard to incorrect projection of the light rays. A ray-tracing-based calibration method for an IIM camera is proposed, to address four errors: MLA decentering, rotational, translational, and subimage-scaling errors. All of these parameters are evaluated using the reference image obtained from the ray-traced white image. The areas and center points of the microlens are estimated using an "8-connected" and a "center-of-gravity" method respectively. The proposed approach significantly improves the rectified-image quality and nonlinear image brightness for an IIM system. Numerical and optical experiments on multiple real objects demonstrate the robustness and effectiveness of our proposed method, which achieves on average a 35% improvement in brightness for an IIM raw image.

• 한국해안해양공학회지
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• 제10권3호
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• pp.109-119
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• 1998

수평 2차원 POM (Princeton Ocean Model)을 바닥마찰과 개방경계조건에 대하여 수정하고, 간석지를 모의하기 위하여 wetting-and-drying 기법을 첨가하여 천수만과 인근연안에 적용하였다. 연구해역의 주된 기작인 조석에 의한 해수유통만을 고려하였다. 본 논문은 천수만 해역에서의 모델 보정과 검증 절차 및 결과를 제시한다. 조석표의 평균 조석 특성을 이용하여 모델영역 전반에 걸쳐 진폭과 위상을 포함하는 조석파의 전파에 대하여 모델을 보장하였고, 보정 결과가 조석파를 잘 재현하였다. 보정된 모델을 1995년 여름 관측된 해수면 변위와 유속에 대한 시계열 자료를 이용하여 검증하였고, 검증 결과가 조석 및 조류를 잘 재현하였다. 보정 및 검증 결과가 본 모델이 천수만 해역에서 조석 현상을 잘 재현할 수 있음을 보여주었다

• Current Optics and Photonics
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• 제8권1호
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• pp.38-44
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• 2024

Under the influence of atmospheric turbulence, a star's point image will shake back and forth erratically, and after exposure the originally small star point will spread into a huge spot, which will affect the ground calibration of the star sensor. To analyze the impact of atmospheric turbulence on the positioning accuracy of the star's center of mass, this paper simulates the atmospheric turbulence phase screen using a method based on a sparse spectrum. It is added to the static-star-simulation device to study the transmission characteristics of atmospheric turbulence in star-point simulation, and to analyze the changes in star points under different atmospheric refractive-index structural constants. The simulation results show that the structure function of the atmospheric turbulence phase screen simulated by the sparse spectral method has an average error of 6.8% compared to the theoretical value, while the classical Fourier-transform method can have an error of up to 23% at low frequencies. By including a simulation in which the phase screen would cause errors in the center-of-mass position of the star point, 100 consecutive images are selected and the average drift variance is obtained for each turbulence scenario; The stronger the turbulence, the larger the drift variance. This study can provide a basis for subsequent improvement of the ground-calibration accuracy of a star sensitizer, and for analyzing and evaluating the effect of atmospheric turbulence on the beam.

• 한국의학물리학회지:의학물리
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• 제2권2호
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• pp.149-154
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• 1991

안과용 $^{90}$ Sr 선원에서 방출하는 $\beta$선의 갯수를 직접 측정함으로써 (전류 측정)표면 선량을 계산하는 방법을 고안하여 실제 교정에 응용하였다. 안과용 $^{90}$ Sr선원에서 방출하는 전체 $\beta$선의 갯수 및 선원의 면적, 전자의 물속에서의 저지능 등을 고려하였다. 선원의 정확한 면적 측정은 필림을 이용하였으며, 평균 저지능은 상기 선원에서 방출되는 $\beta$선의 에너지 스펙트럼을 분석함으로써 얻을 수 있었다. 이 방법과 $^{90}$ Sr으로 교정한 TLD칩을 이용한 교정 방법과의 결과를 비교하였다. 전류 측정 방식에 의한 결과는 63.5$\pm$5.1cGy/sec이었고, TLD칩에 의한 측정 결과는 50.7$\pm$7.3cGy/sec로 오차 범위내에서 일치하였다. 그러나 제작사 보증서에 의하면 46.8$\pm$9.4cGy/sec로 측정값에 비하여 36%의 차이를 보여 주었다.