• Title/Summary/Keyword: Near Infrared Band

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Development of PKNU3: A small-format, multi-spectral, aerial photographic system

  • Lee Eun-Khung;Choi Chul-Uong;Suh Yong-Cheol
    • 대한원격탐사학회지
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    • 제20권5호
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    • pp.337-351
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    • 2004
  • Our laboratory originally developed the compact, multi-spectral, automatic aerial photographic system PKNU3 to allow greater flexibility in geological and environmental data collection. We are currently developing the PKNU3 system, which consists of a color-infrared spectral camera capable of simultaneous photography in the visible and near-infrared bands; a thermal infrared camera; two computers, each with an 80-gigabyte memory capacity for storing images; an MPEG board that can compress and transfer data to the computers in real-time; and the capability of using a helicopter platform. Before actual aerial photographic testing of the PKNU3, we experimented with each sensor. We analyzed the lens distortion, the sensitivity of the CCD in each band, and the thermal response of the thermal infrared sensor before the aerial photographing. As of September 2004, the PKNU3 development schedule has reached the second phase of testing. As the result of two aerial photographic tests, R, G, B and IR images were taken simultaneously; and images with an overlap rate of 70% using the automatic 1-s interval data recording time could be obtained by PKNU3. Further study is warranted to enhance the system with the addition of gyroscopic and IMU units. We evaluated the PKNU 3 system as a method of environmental remote sensing by comparing each chlorophyll image derived from PKNU 3 photographs. This appraisement was backed up with existing study that resulted in a modest improvement in the linear fit between the measures of chlorophyll and the RVI, NDVI and SAVI images stem from photographs taken by Duncantech MS 3100 which has same spectral configuration with MS 4000 used in PKNU3 system.

나노구조 기반 초박형 적외선 차단 필터 (An Ultra-thin IR Cut-off Filter Based on Nanostructures)

  • 양현도;이종권
    • 한국광학회지
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    • 제35권1호
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    • pp.24-29
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    • 2024
  • 본 연구에서는 나노패턴된 금속(Ag)-유전체(PDMS) 다층 기반의 쌍곡선 메타구조를 제안하고 영상 소자용 적외선 차단 필터의 성능에 대해 보고한다. 사각형 모양의 Ag 나노 패턴의 크기와 Ag 나노 패턴을 둘러싼 PDMS의 두께를 최적화함으로써, 제안된 IR 차단 필터가 0.70-1.01 ㎛ 파장 대역의 빛을 99% 차단하면서도 가시광 영역에서 94% 이상의 높은 투과율을 나타냄을 보였다. 차단 파장 대역은 쌍곡선 메타구조의 epsilon-near-zero 파장보다 긴 파장 영역에서 시작하여 Ag 나노 패턴에 의한 플라즈모닉 흡수가 강한 지점에서 끝나게 된다. 근적외선 차단 대역보다 긴 파장 영역에서는 수평으로 인접한 Ag 나노패턴들 사이의 플라즈모닉 커플링 효과로 다시 투과도가 증가됨을 알 수 있다. 이러한 메타구조체는 적외선 차단 필터의 성능을 향상시킬 수 있을 뿐만 아니라 공정 단순화를 통해 초박형 제조가 가능하여, 다양한 평면 광학 및 집적광학 부품들에 적용될 수 있다.

GOCI를 이용한 GOCI-II 근적외 밴드 교차보정 (Cross-Calibration of GOCI-II in Near-Infrared Band with GOCI)

  • 이은경;배수정;안재현;이경상
    • 대한원격탐사학회지
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    • 제39권6_2호
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    • pp.1553-1563
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    • 2023
  • 천리안 해양관측위성 2호기(Geostationary Ocean Color Imager-II, GOCI-II)는 한반도 주변을 포함한 동북아 해역과 전구 영역을 관측하는 해색 위성으로 지난 10년간 운용된 GOCI의 임무를 이어받아 2020년부터 현재까지 운용되고 있다. 본 연구에서는 해색 데이터 산출에 있어 필수 과정인 대기보정 알고리즘을 개선하기 위해 GOCI 영상을 이용한 GOCI-II 근적외 파장(near-infrared, NIR) 밴드의 대리교정을 수행하였다. 이를 위해 NIR 밴드의 대기상층(top-of-atmosphere, TOA) radiance에 대한 교차보정 연구를 수행하였으며, 그 결과로 대리교정 상수를 도출하였다. 본 연구에서 도출된 대리교정 상수를 이용하여 보정한 결과 두 센서의 offset이 감소하였으며, ratio는 745 nm, 865 nm에 대해 각 1.02, 1.04에서 1.0, 0.99로 개선되었다. 이는 두 센서의 일관성이 높아진 것으로 판단된다. 또한, 대기 분자 산란 보정 반사도(Rayleigh-corrected reflectance, 𝜌rc)는 각각 5.62, 9.52% 증가하였다. 이로 인해 745 nm와 865 nm 𝜌rc의 비율의 차이가 발생했으며, 이는 대기보정 알고리즘 내 에어로졸 광 산란 보정 과정을 통해 모든 밴드의 대기보정 결과에 영향을 줄 수 있다. GOCI, GOCI-II 두 위성의 중복되는 운용 기간이 짧아 2021년 3월의 자료만을 사용하였으나, 향후 타위성과의 지속적인 교차보정 연구를 통해 개선이 가능할 것으로 사료된다. 또한 본 연구에서 도출된 NIR 밴드의 대리교정 상수를 적용하여 가시 채널의 대리교정을 수행하고, 해색 산출물의 정확도에 미치는 영향을 분석할 필요가 있다.

척택.어제 침자가 고해상도 적외선 카메라로 관찰한 촌구맥 부위의 온도 Pulsation 변화에 미치는 영향 연구 (Effect of Acupuncture at the LU5(Reinforcement), LU10(Reduction) on the Pulsation Scale of Chon, Gwan and Chuk region using High Resolution Infrared Camera)

  • 나창수;정효상;김지현
    • 대한의용생체공학회:의공학회지
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    • 제32권2호
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    • pp.127-133
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    • 2011
  • Arteria radialis is a branch of the brachial artery extending down the forearm around the wrist where it closes to skin surface. In the oriental medicine, the skin above arteria radialis has an important role because oriental medicine practitioners put their finger tips on the area, and diagnose patient's health conditions by feeling the pulsation of the arterial contraction. The finger tip diagnostic method relies on subjective decision of the practitioner; and there is a need to develop an objective diagnostic modality. The pulsation of the arterial contraction appears not only a movement on the site but also as temperature fluctuation due to pulsatile feeding of warmer blood. The goal of this study is to demonstrate a feasibility of using an infrared camera quantitatively to detect the temperature fluctuation on the skin. Clinical important three different areas, called chon, gwan, chuk, near a wrist where the arteria radialis reaches close to skin surface are marked with small pieces of surgical tape. A high-speed and high-resolution infrared camera with a 3 cm of field of view measures these areas for 10 second at 200 frames per second with a 320*240 pixel size. The pulsatile temperature fluctuation is calculated after passing a band pass filter to remove any stationary temperature over 10 second. The temperature fluctuation of a healthy male volunteer is measured at a room temperature as a control, and is compared with another measurement performed after 20 minutes staying in a room at a 40 degree Celsius. This comparison is repeated for three times, and indicates that the fluctuation increases after staying 20 minutes in the warm room. This increase becomes smaller when the person stays in the warm room with an acupuncture treatment that decreases body temperature. So that an objective diagnostics on the site may become feasible.

IGRINS Mirror Mount Design for Five Flat Mirrors

  • Oh, Jae Sok;Park, Chan;Kim, Kang-Min;Chun, Moo-Young;Yuk, In-Soo;Yu, Young Sam;Oh, Heeyoung;Jeong, Ueejeong;Lee, Hanshin;Jaffe, Daniel T.
    • 천문학회보
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    • 제39권2호
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    • pp.91.2-91.2
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    • 2014
  • A near infrared wide-band high resolution spectrograph, immersion grating infrared spectrometer (IGRINS) has been jointly developed by the Korea Astronomy and Space Science Institute and the University of Texas at Austin. The compact white-pupil design of the instrument optics includes five cryogenic flat mirrors including a slit mirror, an input fold mirror, a dichroic mirror, and H&K camera fold mirrors. In this study, we introduce the optomechanical mount designs of the five cryogenic mirrors. In order to meet the structural stability and thermal requirements of the mount models, we conducted the design work with the aid of 3-dimensional computer modeling and the finite element analysis (FEA) method. We also present the actual fabricated parts and assemblies of the mounts and mirrors as well as their CAD models.

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Extragalactic Sciences from SPICA/FPC-S

  • 정웅섭;;임명신;이형목;이정은;;;;이대희;표정현;박성준;문봉곤;박귀종;박영식;한원용;남욱원
    • 천문학회보
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    • 제38권1호
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    • pp.36.2-36.2
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    • 2013
  • The SPICA (SPace Infrared Telescope for Cosmology & Astrophysics) project is a next-generation infrared space telescope optimized for mid- and far-infrared observation with a cryogenically cooled 3m-class telescope. The focal plane instruments onboard SPICA will enable us to resolve many astronomical key issues from the formation and evolution of galaxies to the planetary formation. The FPC-S (Focal Plane Camera - Sciecne) is a near-infrared instrument proposed by Korea as an international collaboration. Owing to the capability of both low-resolution imaging spectroscopy and wide-band imaging with a field of view of $5^{\prime}{\times}5^{\prime}$, it has large throughput as well as high sensitivity for diffuse light compared with JWST. In order to strengthen advantages of the FPC-S, we propose the studies of probing population III stars by the measurement of cosmic near-infrared background radiation and the star formation history at high redshift by the discoveries of active star-forming galaxies. In addition to the major scientific targets, to survey large area opens a new parameter space to investigate the deep Universe. The good survey capability in the parallel imaging mode allows us to study the rare, bright objects such as quasars, bright star-forming galaxies in the early Universe as a way to understand the formation of the first objects in the Universe, and ultra-cool brown dwarfs. Observations in the warm mission will give us a unique chance to detect high-z supernovae, ices in young stellar objects (YSOs) even with low mass, the $3.3{\mu}$ feature of shocked circumstance in supernova remnants. Here, we report the current status of SPICA/FPC project and its extragalactic sciences.

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MgGa$_2$Se$_4$신반도체 단결정을 사용한 광전도도 소자 제작에 관한 연구 (A Study on the Photoconductive Cell Production of New Semiconductor Using MgGa$_2$Se$_4$Single Crystals)

  • 김형곤;김형윤;이광석;이기형
    • 한국통신학회논문지
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    • 제17권1호
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    • pp.58-67
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    • 1992
  • MgGa2Se4 및 MgGa2Se4 : Co2+단결정을 bridgman 방법으로 성장하여 광흡수와 광발광을 가시광 영역과 근적외선 영역에서 조사하였다. 광흡수 스펙트럼은 MgGa2Se4단결정의 Td Symmetry를 갖는 host lattice에 점유하여 바닥상태와 여기상태의 Co2+ ion 에너지 ㅣlevel간 전자전이에 의해서 760nm, 1640nm, 그리고 2500nm에서 3개의 흡수피크를 관측하였다. 광발광 스펙트럼에서 이 단결정은 가시광 발광ㄸ들을 관찰하였다.가시영역의 발광 band들은 에너지 준위도에서 제안된 바와 같이 자전자대의 우의 꼭대기 acceptor 준위에서 전도대 아래의 밑에 분포된 trap으로부터 끊임없이 전자전에 의한다고 볼수 있다. 한편, 이들은 적외선 발광 band가 deep level에서 acceptor level부터 전자전이에 기인한다고 고려할 수 있다. 광전이의 mechanism은 MgGa2Se4 결정의 에너지 diagram의 항으로 잘 설명되고 있다.

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IGRINS : Mirror Mounts Optomechanical Design

  • ;박찬;이성호;;이한신;오희영;정화경;육인수;;김강민;천무영
    • 천문학회보
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    • 제36권2호
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    • pp.155.1-155.1
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    • 2011
  • The Korea Astronomy and Space Science Institute (KASI) and the Department of Astronomy at the University of Texas at Austin (UT) are developing a near infrared wide-band high resolution spectrograph, IGRINS (Immersion Grating Infrared Spectrograph). The white-pupil design of the instrument optics uses 7 cryogenic mirrors including 3 aspherical off-axis collimators and 4 flat fold mirrors. Two of the 3 collimators are H- and K-band pupil transfer mirrors and they are designed as compensators for the system alignment in each channel. Therefore, their mount design will be one of the most sensitive parts in the IGRINS optomechanical system. The other flat fold mirrors are designed within the limited area. Each of those includes the features of 3 axial hard points and 2 radial hard points with one spring plunger in order for the proper deflection of the mirror. The design work will include the computer-aided 3D modeling and finite element analysis (FEA) to optimize the structural stability and the thermal behavior of the mount models. The mount body will also include a tip-tilt and translation adjustment mechanism to be used as the alignment compensators.

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SPECTROSCOPIC AND CHEMOMETRIC ANALYSIS OF SW-NIR SPECTRA OF SUGARS AND FRUITS

  • Golic, Mirta;Walsh, Kerry;Lawson, Peter
    • 한국근적외분광분석학회:학술대회논문집
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    • 한국근적외분광분석학회 2001년도 NIR-2001
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    • pp.1133-1133
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    • 2001
  • Fruit sweetness, as indexed by total soluble solids (TSS), and fruit acidity are key factors in the description of the fruit eating quality. Our group has been using short wave NIR spectroscopy (SW-NIR; 700-1100 nm) in combination with chemometric methods (PLS and MLR) for the non-invasive determination of the fruit eating quality (1,2). In order to further improve calibration performance, we have investigated SW-NIR spectra of sucrose and D-glucose. In previous reports on the band assignment for these sugars in the 1100-2500 nm spectral region (3-7), it has been established that change in concentration, temperature and physical state of sugars reflects on the shape and position of the spectral bands in the whole NIR region(5-7). The effect of change in concentration and temperature of individual sugar solutions and sugar spiked Juice samples was analysed using combined spectroscopic (derivative, difference, 2D spectroscopy) and linear regression chemometric (PLS, MLR) techniques. The results have been compared with the spectral data of a range of fruit types, varying in TSS content and temperature. In the 800-950 nm spectral region, the B-coefficients for apples, peaches and nectarines resemble those generated in a calibration of pure sucrose in water (Fig. 1). As expected, these fruits exhibit better calibration and prediction results than those in which the B-coefficients were poorly related to those for sugar.(Figure omitted).

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IMAGING SPECTROMETRY FOR DETECTING FECES AND INGESTA ON POULTRY CARCASSES

  • Park, Bo-Soon;William R.Windham;Kurt C.Lawrence;Smith, Douglas-P
    • 한국근적외분광분석학회:학술대회논문집
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    • 한국근적외분광분석학회 2001년도 NIR-2001
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    • pp.3106-3106
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    • 2001
  • Imaging spectrometry or hyperspectral imaging is a recent development that makes possible quantitative and qualitative measurement for food quality and safety. This paper presents the research results that a hyperspectral imaging system can be used effectively for detecting fecal (from duodenum, cecum, and colon) and ingesta contamination on poultry carcasses from the different feed meals (wheat, mile, and corn with soybean) for poultry safety inspection. A hyperspectral imaging system has been developed and tested for the identification of fecal and ingesta surface contamination on poultry carcasses. Hypercube image data including both spectral and spatial domains between 430 and 900 nm were acquired from poultry carcasses with fecal and ingesta contamination. A transportable hyperspectral imaging system including fiber optically fabricated line lights, motorized lens control for line scans, and hypercube image data from contaminated carcasses with different feeds are presented. Calibration method of a hyperspectral imaging system is demonstrated using different lighting sources and reflectance panels. Principal Component and Minimum Noise Fraction transformations will be discussed to characterize hyperspectral images and further image processing algorithms such as image band ratio of dual-wavelength images and its histogram stretching with thresholding process will be demonstrated to identify fecal and ingesta materials on poultry carcasses. This algorithm could be further applied for real-time classification of fecal and ingesta contamination on poultry carcasses in the poultry processing line.

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