• 제목/요약/키워드: Infrared: imaging

검색결과 767건 처리시간 0.032초

GaAs 웨이퍼의 대역단 영상에 대한 정량적 해석 (Quantitative Analysis on Near Band Edge Images in GaAs Wafer)

  • 강성준;나철훈
    • 한국정보통신학회논문지
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    • 제21권5호
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    • pp.861-868
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    • 2017
  • 도핑 되지 않은 반 절연 LEC GaAs내의 EL2와 얕은 준위 분포를 영상화하기 위해 대역단 적외선 영상 기법을 활용했다. 대역단 적외선 투사 매핑에 근거한 본 기법은 분석 속도가 빠르고 비파괴적인 방법이다. EL2 흡수 영상이 콘트라스트 반전되는 대역단 부근에 대한 정량적인 해석은 아직 보고되지 않고 있다. 본 논문은 대역단 부근에서 영상의 특정 부분(cell, wall)에 대한 포토퀀칭 메커니즘의 스펙트럼-, 공간- 및 온도- 종속성을 논하고 있다. 결함 부분별(EL2w, EL2b)로 포토퀀칭 개시점이 다른 것은 불순물 종류의 차이로 인한 서로 다른 전기적 작용에 기인한 것으로 해석할 수 있다. 전위(dislocation) 밀도가 높은 곳에서는 EL2b 밀도는 약간 적은 반면 EL2w 밀도는 보다 많다는 것을 정량적 해석으로부터 확인 했다.

OPTICAL SURVEY WITH KMTNET FOR DUSTY STAR-FORMING GALAXIES IN THE AKARI DEEP FIELD SOUTH

  • JEONG, WOONG-SEOB;KO, KYEONGYEON;KIM, MINJIN;KO, JONGWAN;KIM, SAM;PYO, JEONGHYUN;KIM, SEONG JIN;KIM, TAEHYUN;SEO, HYUN JONG;PARK, WON-KEE;PARK, SUNG-JOON;KIM, MIN GYU;KIM, DONG JIN;CHA, SANG-MOK;LEE, YONGSEOK;LEE, CHUNG-UK;KIM, SEUNG-LEE;MATSUURA, SHUJI;PEARSON, CHRIS;MATSUHARA, HIDEO
    • 천문학회지
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    • 제49권5호
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    • pp.225-232
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    • 2016
  • We present an optical imaging survey of AKARI Deep Field South (ADF-S) using the Korea Microlensing Telescope Network (KMTNet), to find optical counterparts of dusty star-forming galaxies. The ADF-S is a deep far-infrared imaging survey region with AKARI covering around 12 deg2, where the deep optical imaging data are not yet available. By utilizing the wide-field capability of the KMTNet telescopes (~4 deg2), we obtain optical images in B, R and I bands for three regions. The target depth of images in B, R and I bands is ~24 mag (AB) at 5σ, which enables us to detect most dusty star-forming galaxies discovered by AKARI in the ADF-S. Those optical datasets will be helpful to constrain optical spectral energy distributions as well as to identify rare types of dusty star-forming galaxies such as dust-obscured galaxy, sub-millimeter galaxy at high redshift.

과학기술위성 3호 운영개념 (STSAT-3 Operations Concept)

  • 이승헌;박종오;이승우;정태진;이대희;이준호
    • 항공우주기술
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    • 제10권2호
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    • pp.29-36
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    • 2011
  • 과학기술위성 3호는 우리별 위성 시리즈와 과학기술위성 1호, 2호를 잇는 소형위성으로 첨단 위성체 핵심 기술 선행연구, 첨단 우주 및 지구 과학 탑재체 개발, 우주분야 인력 양성 등의 다양한 역할을 수행한다. 과학기술위성의 주탑재체는 다목적 적외선 영상시스템으로 우리은하와 황도극지방을 관측하여 우주의 기원을 연구한다. 다목적 적외선 영상시스템에는 국산 적외선 센서의 우주검증을 위해 지표면의 적외선 영상 획득 임무도 추가되었다. 부탑재체는 초소형 영상 분광기로서 농작물의 작황, 댐의 수질 예측 모델, 에어로졸 광학 두께 측정 연구 등에 활용된다. 본 논문에서는 2012년 말에 발사되어 주어진 임무기간 동안 과학기술위성 3호의 다양한 임무 수행을 위한 운영개념을 설명한다.

Hybrid 렌즈를 이용한 비냉각 열상장비 광학계 설계 및 분석 (Design and Analysis of an Optical System for an Uncooled Thermal-imaging Camera Using a Hybrid Lens)

  • 옥창민;공현배;박현우
    • 한국광학회지
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    • 제28권5호
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    • pp.241-249
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    • 2017
  • 본 논문에서는 $7.7{\mu}m$에서 $12.8{\mu}m$ 파장 대역에 적용 가능한 비냉각 열상장비 광학계를 설계 및 분석 하였다. 최적화 과정을 통하여 설계된 원적외선 광학계의 유효초점거리는 5.44 mm를 가지며, 4면의 비구면과 2면의 회절면을 포함하였다. 광학계의 F/수는 F/1.2로 설정하였고, 시야각은 $90^{\circ}{\times}67.5^{\circ}$가 되도록 하였다. 회절면이 적용된 hybrid 렌즈를 이용하여 보다 효율적으로 고차 수차가 보정되도록 하였고, 이때 발생되는 회절 특성은 scalar 회절 효율을 이용하여 평가하였다. 또한 hybrid 렌즈에서 발생되는 회절 현상에 의한 통합 회절효율을 예측하고 배경잡음에 의한 MTF 저하를 고려하였다. 원적외선 광학계의 온도 변화에 따른 보상은 광학식 비열화를 이용하여 광학계의 MTF 성능이 초점 심도 내에서 유지되도록 하였다. 결론적으로 비냉각 열상장비에 효율적으로 적용 가능한 광학설계 결과를 얻었다.

The Characterization of Anti-HER-2/neu Monoclonal Antibody using Different in vivo Imaging Techniques

  • Moon, Cheol;Kim, Eun Jung;Choi, Dan Bee;Kim, Byoung Soo;Kim, Sa Hyun;Choi, Tae Hyun
    • 대한의생명과학회지
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    • 제21권1호
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    • pp.23-31
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    • 2015
  • Recently, specific antibodies have been used extensively to diagnose and treat various diseases. It is essential to assess the efficacy and specificity of antibodies, especially the in vivo environment. Anti-HER-2/neu mAb was evaluated as a possible transporting agent for radioimmunotherapy. The monoclonal antibody was successfully radio-labeled with $^{131}I$. In vitro binding assays were performed to confirm its targeting ability using another radio-iodine, $^{125}I$. Binding percentage of $^{125}I$ labeled anti-HER-2/neu mAb in HER-2/neu expressing CT-26 cells was found to be 4.5%, whereas the binding percentage of $^{125}I$ labeled anti-HER-2/neu mAb in wild-type CT-26 was only 0.45%. In vivo images were obtained and analyzed through $\gamma$-camera and an optical fluorescent modality, IVIS-200. $\gamma$-camera images showed that $^{131}I$ labeled anti-HER-2/neu mAb accumulated in HER-2/neu CT-26 tumors. Optical imaging based on near infrared fluorescence labeled anti-HER-2/neu mAb showed higher fluorescence intensities in HER-2/neu CT-26 tumors than in wild-type CT-26 tumors. Anti-HER-2/neu mAb was found to specifically bind to its receptor expressing tumor. Our study demonstrates that in vivo imaging technique is a useful method for the evaluation of an antibody's therapeutic and diagnostic potentials.

테라헤르츠 이미징 기술 및 그 응용 분야 (Terahertz Imaging Technology and Applications)

  • 김무건;이의수;박동우;최다혜;이일민;신준환;김영호;김정수;조진철;김영훈;곽동용;박경현
    • 전자통신동향분석
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    • 제36권3호
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    • pp.97-105
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    • 2021
  • The terahertz wave (THz wave) is a band between infrared and microwaves and is defined as an electromagnetic wave having a frequency of 0.1 to 10 THz band. THz waves have the property of transmitting nonpolar materials, which the visible light cannot be transmitted, such as ceramics, plastics, and paper; and the photon energy is low, such as several meV. For this reason, non-destructive testing equipment based on THz imaging technology can be applied to the industrial field. Recently, THz imaging technology was applied in wide industrial fields, such as automobiles, batteries, food, medical, and security, and being actively studied. In this paper, we describe the research trends of terahertz imaging technology and experimental results. Furthermore, we summarize the recent commercialized terahertz camera. Finally, we present the research results in the field of the human security scanner system.

Construction of a Ginsenoside Content-predicting Model based on Hyperspectral Imaging

  • Ning, Xiao Feng;Gong, Yuan Juan;Chen, Yong Liang;Li, Hongbo
    • Journal of Biosystems Engineering
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    • 제43권4호
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    • pp.369-378
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    • 2018
  • Purpose: The aim of this study was to construct a saponin content-predicting model using shortwave infrared imaging spectroscopy. Methods: The experiment used a shortwave imaging spectrometer and ENVI spectral acquisition software sampling a spectrum of 910 nm-2500 nm. The corresponding preprocessing and mathematical modeling analysis was performed by Unscrambler 9.7 software to establish a ginsenoside nondestructive spectral testing prediction model. Results: The optimal preprocessing method was determined to be a standard normal variable transformation combined with the second-order differential method. The coefficient of determination, $R^2$, of the mathematical model established by the partial least squares method was found to be 0.9999, while the root mean squared error of prediction, RMSEP, was found to be 0.0043, and root mean squared error of calibration, RMSEC, was 0.0041. The residuals of the majority of the samples used for the prediction were between ${\pm}1$. Conclusion: The experiment showed that the predicted model featured a high correlation with real values and a good prediction result, such that this technique can be appropriately applied for the nondestructive testing of ginseng quality.

Optical Design of a Snapshot Nonmydriatic Fundus-imaging Spectrometer Based on the Eye Model

  • Zhao, Xuehui;Chang, Jun;Zhang, Wenchao;Wang, Dajiang;Chen, Weilin;Cao, Jiajing
    • Current Optics and Photonics
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    • 제6권2호
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    • pp.151-160
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    • 2022
  • Fundus images can reflect ocular diseases and systemic diseases such as glaucoma, diabetes mellitus, and hypertension. Thus, research on fundus-detection equipment is of great importance. The fundus camera has been widely used as a kind of noninvasive detection equipment. Most existing devices can only obtain two-dimensional (2D) retinal-image information, yet the fundus of the human eye also has spectral characteristics. The fundus has many pigments, and their different distributions in the eye lead to dissimilar tissue penetration for light waves, which can reflect the corresponding fundus structure. To obtain more abundant information and improve the detection level of equipment, a snapshot nonmydriatic fundus imaging spectral system, including fundus-imaging spectrometer and illumination system, is studied in this paper. The system uses a microlens array to realize snapshot technology; information can be obtained from only a single exposure. The system does not need to dilate the pupil. Hence, the operation is simple, which reduces its influence on the detected object. The system works in the visible and near-infrared bands (550-800 nm), with a volume less than 400 mm × 120 mm × 75 mm and a spectral resolution better than 6 nm.

An exosolar planetary system N-body simuInfrared Spectro-Photometric Survey in Space: NISS and SPHEREx Missions

  • Jeong, Woong-Seob;Kim, Minjin;Im, Myungshin;Lee, Jeong-Eun;Pyo, Jeonghyun;Song, Yong-Seon;Park, Sung-Joon;Moon, Bongkon;Lee, Dae-Hee;Park, Won-Kee;Jo, Youngsoo;Lee, Duk-Hang;Ko, Kyeongyeon;Kim, Il-Joong;Park, Youngsik;Yang, Yujin;Ko, Jongwan;Lee, Hyung Mok;Shim, Hyunjin;Shin, Goo-Hwan;Chae, Jangsoo;Matsumoto, Toshio
    • 천문학회보
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    • 제43권1호
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    • pp.47.1-47.1
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    • 2018
  • The NISS (Near-infrared Imaging Spectrometer for Star formation history) onboard NEXTSat-1 have successfully developed by KASI. The capability of both imaging and spectroscopy is a unique function of the NISS. At first, it have realized the low-resolution spectroscopy (R~20) with a wide field of view of $2{\times}2deg$. in a wide near-infrared range from 0.95 to $2.5{\mu}m$. The major scientific mission is to study the cosmic star formation history in local and distant universe. It will also demonstrate the space technologies related to the infrared spectro-photometry in space. Now, the NISS is ready to launch in late 2018. After the launch, the NISS will be operated during 2 years. As an extension of the NISS, the SPEHREx (Spectro-Photometer for the History of the Universe Epoch of Reionization, and Ices Explorer) is the NASA MIDEX (Medium-class Explorer) mission proposed together with KASI (PI Institute: Caltech). It will perform the first all-sky infrared spectro-photometric survey to probe the origin of our Universe, to explore the origin and evolution of galaxies, and to explore whether planets around other stars could harbor life. Compared to the NISS, the SPHEREx is designed to have much more wide FoV of $3.5{\times}11.3deg$. as well as wide spectral range from 0.75 to $5.0{\mu}m$. After passing the first selection process, the SPHEREx is under the Phase-A study. The final selection will be made in the end of 2018. Here, we report the status of the NISS and SPHEREx missions.

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Automatic Detection of Malfunctioning Photovoltaic Modules Using Unmanned Aerial Vehicle Thermal Infrared Images

  • Kim, Dusik;Youn, Junhee;Kim, Changyoon
    • 한국측량학회지
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    • 제34권6호
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    • pp.619-627
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    • 2016
  • Cells of a PV (photovoltaic) module can suffer defects due to various causes resulting in a loss of power output. As a malfunctioning cell has a higher temperature than adjacent normal cells, it can be easily detected with a thermal infrared sensor. A conventional method of PV cell inspection is to use a hand-held infrared sensor for visual inspection. The main disadvantages of this method, when applied to a large-scale PV power plant, are that it is time-consuming and costly. This paper presents an algorithm for automatically detecting defective PV panels using images captured with a thermal imaging camera from an UAV (unmanned aerial vehicle). The proposed algorithm uses statistical analysis of thermal intensity (surface temperature) characteristics of each PV module to verify the mean intensity and standard deviation of each panel as parameters for fault diagnosis. One of the characteristics of thermal infrared imaging is that the larger the distance between sensor and target, the lower the measured temperature of the object. Consequently, a global detection rule using the mean intensity of all panels in the fault detection algorithm is not applicable. Therefore, a local detection rule was applied to automatically detect defective panels using the mean intensity and standard deviation range of each panel by array. The performance of the proposed algorithm was tested on three sample images; this verified a detection accuracy of defective panels of 97% or higher. In addition, as the proposed algorithm can adjust the range of threshold values for judging malfunction at the array level, the local detection rule is considered better suited for highly sensitive fault detection compared to a global detection rule. In this study, we used a panel area extraction method that we previously developed; fault detection accuracy would be improved if panel area extraction from images was more precise. Furthermore, the proposed algorithm contributes to the development of a maintenance and repair system for large-scale PV power plants, in combination with a geo-referencing algorithm for accurate determination of panel locations using sensor-based orientation parameters and photogrammetry from ground control points.