• 한국군사과학기술학회지
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• 제17권4호
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• pp.521-530
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• 2014

In this paper, the glint effect of maritime target to a radar system was analyzed by simulation and field test with a barge and corner reflectors. From the experiment, we proposed a glint measurement method of a real maritime target and it was indicated that the glint effect between the simulation results and real measurement is similar. Also it was founded that the glint effect is related to the relative amount of RCS(Radar Cross Section) difference among major scattering point and minor scattering points. Finally, the experiment showed the glint effects of the rotating barge with some different combinations of scattering points.

• 대한임베디드공학회논문지
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• 제12권1호
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• pp.27-34
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• 2017

The signal transmitted from radar is not reflected from a single point when the signal reflected by complex target. Resultantly, the amplitude and phase of the received signal can be changed because the target has lots of scatterers. The changes of the amplitude and the phase mean Glint and RCS, respectively. Although the Glint and RCS that caused by the same scatters are uncorrelated, however, they are not independent completely. Therefore, this paper proposes a method for generating the Glint and RCS by using same random number generator. And the time correlations of the Glint and RCS are respectively implemented in frequency domain by using each power spectral density of them.

• 대한원격탐사학회지
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• 제31권4호
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• pp.281-291
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• 2015

Sun glint correction methods of hyperspectral data that have been developed so far have not considered the various situations and are often adequate for only certain conditions. Also there is an inaccurate assumption that the signal in NIR wavelength is zero. Therefore, this study attempts to analyze the NIR spectral properties of sun glint effect in coastal waters. For the analysis, CASI-1500 airborne hyperspectral data, bathymetry data and in-situ data obtained at coastal area near Sin-Cheon, Jeju Island, South Korea were used. The spectral characteristics of radiance and reflectance at the five NIR wavelengths (744 nm, 758 nm, 772 nm, 786 nm, and 801 nm) are analyzed by using various statistics, spatial and spectral variation of sun-glinted area under conditions of the bottom types of benthos, barren rocks and sand with similar water depth. Through the quantitative analysis, we found that the relation of water depth or bottom type with sun glint is relatively less which is a similar result with the previous studies. However the sun glint are distributed similarly with the patterns of the direction of wave propagation. It is confirmed that the areas with changed direction of wave propagation were not affected by the sun glint. The spatial and spectral variations of radiance and reflectance are mainly caused by the effect of sun glint and waves. The radiance or reflectance of more sun-glinted areas are increased approximately 1.5 times and the standard deviations are also increased three times compared to the less sun glinted areas. Through this study, the further studies of sun glint correction method in coastal water using the patterns of wave propagation and diffraction will be placed.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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• pp.387-392
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• 1998

To establish a monthly data collection planning for the Ocean Scanning Multispectral Imager (OSMI), we have examined the global patterns of three impacting factors: pigment concentration, cloud cover, and sun glint. Other than satellite mission constraints (e.g., duty cycle), these three factors are considered critical for the OSMI data collection. The Nimbus-7 Coastal Zone Color Scanner (CZCS) monthly mean products and the International Satellite Cloud Climatology Project (ISCCP) monthly mean products (C2) were used for the analysis of pigment concentration and cloud cover distributions, respectively. And the monthly simulated patterns of sun glint were produced by performing the OSMI orbit prediction and the calculation of sun glint radiances at the top-of-atmosphere (TOA). Using monthly statistics (mean and/or standard deviation) of each factor in the above for a given 10$^{\circ}$ latitude by 10$^{\circ}$ longitude grid, we generated the priority map for each month. The priority maps of three factors for each month were subsequently superimposed to visualize the impact of three factors in all. The initial results illustrated that a large part of oceans in the summer hemisphere was classified into the low priority regions because of seasonal changes of clouds and sun illumination. Sensitivity tests were performed to see how cloud cover and sun glint affect the priority determined by pigment concentration distributions, and consequently to minimize their seasonal effects upon the data collection planning.

• 제어로봇시스템학회논문지
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• 제7권8호
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• pp.711-715
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• 2001

In this paper, an effective filter structure for filtering of target glint in tracking radar systems is used to improve the performance of CLOS(Command to Line-Of-Sight) guidance. The filter decouples range and angel channels to that it has a sound mathematical basis as well as computation efficiency as applied to the IMM algorithm. The effective filter structure in conjunction with CLOS guidance is tested by a series of simulation runs and it is shown to have superior performance compared with the other filter structures.

• Journal of Astronomy and Space Sciences
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• 제22권3호
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• pp.263-272
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• 2005

2008년 발사 예정인 통신해양기상위성의 해양 관측자료 분석에 적용할 해수면에 나타나는 태양광 반사점의 위치를 찾아주는 알고리즘을 연구하였다. 태양-위성-지구의 기하학적 위치를 고려한 위성과 태양의 방위각과 고도각의 계산을 통해 비선형 방정식을 유도하였고, 뉴톤-랩슨 수치 방법을 이용하여 해를 구하였다. 통신해양기상위성이 동경 $116.2^{\circ}E$ 혹은 $128.2^{\circ}E$에 위치하게 될 경우 위도 ${\pm}10^{\circ}(N-S)$와 경도 사이에 태양광 반사점이 분포하는 것을 알 수 있었다. 남반구의 낮 동안 태양광 반사점의 경로는 북극을 향해 휘어있고 반대로 북반구의 태양광 반사점의 경로는 남극을 향하는 분포 패턴을 도출해 내었다. 다양한 영상 센서를 가진 정지궤도 위성들의 태양광 반사점의 위치예측과 그와 관련된 연구를 수행하는데 있어 본 논문에서 연구한 알고리즘을 이용할 수 있다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2001년도 합동 추계학술대회 논문집 정보 및 제어부문
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• pp.26-29
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• 2001

In a target tracking problem the radar glint noise has non-Gaussian heavy-tailed distribution and will seriously affect the target tracking performance. In most nonlinear situations an Extended Robust Kalman Filter(ERKF) can yield acceptable performance as long as the noises are white Gaussian. However, an Extended Robust $H_{\infty}$ Filter (ERHF) can yield acceptable performance when the noises are Laplacian. In this paper, we use the Interacting Multiple Model(IMM) estimator for the problem of target tracking with glint noise. In the IMM method, two filters(ERKF and ERHF) are used in parallel to estimate the state. Computer simulations of a real target tracking shows that hybrid filter used the IMM algorithm has superior performance than a single type filter.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2001년도 하계학술대회 논문집 D
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• pp.1961-1963
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• 2001

In a target tracking problem, the radar glint noise has non-Gaussian heavy-tailed distribution and will seriously affect the target tracking performance. In this study, an extended robust $H_{\infty}$ was developed which can significantly improve the tracking performance when glint noise is present. Through the computer simulations, the proposed filter showed superior and robust tracking performance compared with other extended Kalman filters.

• 한국정보통신학회논문지
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• 제18권10호
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• pp.2417-2426
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• 2014

간접 시선 추적 시스템은 적외선 조명을 각막에 반사시켜 그 모습을 카메라로 촬영하여 얻은 이미지에서 시선을 계산한다. 적외선 조명이 각막에 반사되어 이미지에 나타난 점을 글린트라고 한다. 최근 간접 추적 시스템은 머리의 움직임에 민감하지 않고 캘리브레이션 과정을 거치지 않도록 하기 위해 여러 개의 적외선 조명, 즉 여러개의 글린트를 사용하는 경우가 많다. 하지만 실험 도중 글린트의 일부가 보이지 않을 수 있는데, 이러한 경우 해당 프레임에서는 시선 계산을 할 수 없게 된다. 본 논문에서는 여러 개의 적외선 조명을 사용하는 시선 추적 시스템에서 여러 가지 이유로 유실되거나 인식이 어려운 글린트의 모습을 살펴본 후, 인식이 가능한 나머지 글린트 위치를 이용하여 이러한 글린트의 위치를 복원하는 알고리즘을 제안한다. 이 알고리즘을 통해 시선 추적 시 유효한 이미지 프레임의 개수를 증가 시키고, 복원 단계에서 글린트의 위치 변형 모델을 이용하여 글린트의 왜곡 또한 보정하여 시선 추적 결과의 오차도 줄일 수 있다.

• 대한원격탐사학회지
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• 제14권3호
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• pp.277-284
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• 1998

해색관측센서 (OSMI)의 월별 자료수집계획을 수립하기 위해 색소농도, 운량 및 태양반사의 세가지 영향요소에 대한 전구분포가 검토되었다. 위성의 임무 제한조건 (예, 임무주기)을 제외한 이들 세 요소들은 OSMI 자료수집에 매우 중요한 것으로 간주된다. Nimbus-7 CZCS 월평균 자료 및 ISCCP 월평균 자료가 색소농도 및 운량 분포 분석에 각각 사용되었다. 그리고 태양반사의 월별 모사분포는 OSMI 궤도예측 및 대기 상층부 태양반사 레이디언스 계산을 수행함으로 얻어졌다. 주어진 경위도 $10^{\circ}$격자에 대한 상기 각 요소의 월별 통계자료 (월평균 혹은 표준편차)를 이용해 월별 우선순위 도를 생성시켰다. 이어서 세 요소의 중복효과를 보기위해 각 달의 세 요소에 대한 우선순위 도를 중첩 시켰다. 초기결과는 하반구의 대부분이 구름과 태양반사의 계절변화로 인해 우선순위가 낮은 지역으로 분류됨을 보였다. 서로 다른 분류세트에 대한 민감도 시험을 하여 구름과 태양반사의 계절변화가 강건함을 보였다.