• 한국방송∙미디어공학회:학술대회논문집
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• 한국방송∙미디어공학회 2019년도 추계학술대회
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• pp.233-234
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• 2019

We propose a novel algorithm for detecting ship wake trails in optical images of the maritime environment. The proposed algorithm first removes the sky region by localizing the horizon to prevent false wake trails detection. Then, a feature map is computed by employing brightness distortion and chromatic distortion. The feature map is thresholded to obtain a rough estimate of wake trails. Finally, the wake map is refined using the shape prior information. Experimental results show that the proposed algorithm can effectively detect wake trails in images.

• 대기
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• 제29권1호
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• pp.61-74
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• 2019

To investigate the observational environment, sky line and skyview factor (SVF) are calculated using a digital elevation model (DEM; 10 m spatial resolution) and 3 dimensional (3D) sky image at radiation site, Gangneung-Wonju National University (GWNU). Solar radiation is calculated using GWNU solar radiation model with and without the sky line and the SVF retrieved from the 3D sky image and DEM. When compared with the maximum sky line elevation from Skyview, the result from 3D camera is higher by $3^{\circ}$ and that from DEM is lower by $7^{\circ}$. The SVF calculated from 3D camera, DEM and Skyview is 0.991, 0.998, and 0.993, respectively. When the solar path is analyzed using astronomical solar map with time, the sky line by 3D camera shield the direct solar radiation up to $14^{\circ}$ with solar altitude at winter solstice. The solar radiation is calculated with minutely, and monthly and annual accumulated using the GWNU model. During the summer and winter solstice, the GWNU radiation site is shielded from direct solar radiation by the west mountain 40 and 60 minutes before sunset, respectively. The monthly difference between plane and real surface is up to $29.18M\;m^{-2}$ with 3D camera in November, while that with DEM is $4.87M\;m^{-2}$ in January. The difference in the annual accumulated solar radiation is $208.50M\;m^{-2}$ (2.65%) and $47.96M\;m^{-2}$ (0.63%) with direct solar radiation and $30.93M\;m^{-2}$ (0.58%) and $3.84M\;m^{-2}$ (0.07%) with global solar radiation, respectively.

• 천문학논총
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• 제27권4호
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• pp.111-116
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• 2012

Far-infrared observations provide crucial data for the investigation and characterisation of the properties of dusty material in the Interstellar Medium (ISM), since most of its energy is emitted between ~ 100 and $200{\mu}m$. We present the first all-sky image from a sensitive all-sky survey using the Japanese AKARI satellite, in the wavelength range $50-180{\mu}m$. Covering > 99% of the sky in four photometric bands with four filters centred at $65{\mu}m$, $90{\mu}m$, $140{\mu}m$, and $160{\mu}m$ wavelengths, this achieved spatial resolutions from 1 to 2 arcmin and a detection limit of < 10 MJy $sr^{-1}$, with absolute and relative photometric accuracies of < 20%. All-sky images of the Galactic dust continuum emission enable astronomers to map the large-scale distribution of the diffuse ISM cirrus, to study its thermal dust temperature, emissivity and column density, and to measure the interaction of the Galactic radiation field and embedded objects with the surrounding ISM. In addition to the point source population of stars, protostars, star-forming regions, and galaxies, the high Galactic latitude sky is shown to be covered with a diffuse filamentary-web of dusty emission that traces the potential sites of high latitude star formation. We show that the temperature of dust particles in thermal equilibrium with the ambient interstellar radiation field can be estimated by using $90{\mu}m$, $140{\mu}m$, and $160{\mu}m$ data. The FIR AKARI full-sky maps provide a rich new data set within which astronomers can investigate the distribution of interstellar matter throughout our Galaxy, and beyond.

• 천문학회보
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• 제42권2호
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• pp.55.1-55.1
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• 2017

HectoMAP is a dense redshift survey of red galaxies covering a 53 square degree strip of the northern sky, and Horizon Run 4 is one of the densest and largest cosmological simulations based on the standard Lambda cold dark matter model. We use HectoMAP and Horizon Run 4 to compare the physical properties of observed large-scale structures with simulated ones in the redshift range 0.22

• 천문학회지
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• 제29권spc1호
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• pp.125-126
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• 1996

Beijing-Arizona-Taipei-Connecticut (BATC) survey is a long term project to map the spectral energy distribution of various objects using 15 intermediate band filters and aims to cover about 450 sq degrees of northern sky. The SED information, combined with image structure information, is used to classify objects into several stellar and galaxy categories as well as QSO candidates. In this paper, we present a preliminary setup of robust data reduction procedure recently developed at NCU and also briefly discuss general classification scheme: redshift estimate, and automatic detection of variable objects.

• 대기
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• 제31권5호
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• pp.525-537
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• 2021

Black ices on road surfaces in winter tend to cause severe and terrible accidents. It is very difficult to detect black ice events in advance due to their localities as well as sensitivities to surface and upper meteorological variables. This study develops a methodology to detect the road sections vulnerable to black ice with the use of road surface temperature data obtained from a mobile road weather observation vehicle. The 7 experiments were conducted on the route from Nam-Wonju IC to Nam-Andong IC (132.5 km) on the Jungang Expressway during the period from December 2020 to February 2021. Firstly, temporal road surface temperature data were converted to the spatial data with a 50 m resolution. Then, the spatial road surface temperature was normalized with zero mean and one standard deviation using a simple normalization, a linear de-trend and normalization, and a low-pass filter and normalization. The resulting road thermal map was calculated in terms of road surface temperature differences. A road ice index was suggested using the normalized road temperatures and their horizontal differences. Road sections vulnerable to black ice were derived from road ice indices and verified with respect to road geometry and sky view, etc. It was found that black ice could occur not only over bridges, but also roads with a low sky view factor. These results are expected to be applicable to the alarm service for black ice to drivers.

• 천문학논총
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• 제27권4호
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• pp.263-264
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• 2012

We present the properties of dust and the near-infrared spectral features in nearby early-type galaxies. The properties of dust are obtained from the AKARI far-infrared all-sky survey diffuse map. The AKARI/IRC is used for the near-infrared spectra. We improve spectral data with the new dark subtraction method on the basis of the knowledge acquired in our laboratory experiments of the engineering-model detector for the IRC. We have succeeded in fitting the continuum by a power-law function and detecting CO and SiO absorption features in early-type galaxy spectra. Comparing the properties of dust and near-infrared spectral features, we find that the power-law slope depends on dust temperature, but not on the dust mass, which suggests that low-luminosity AGNs may contribute to the changes in the power-law slope and dust temperature.

• 지구물리
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• 제9권4호
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• pp.361-369
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• 2006

본 연구에서는 AHRS IMU 센서를 이용하여 동적 위치 결정을 위해 초기화 시험을 실시하여 회귀분석을 통해 시간에 대한 이동체의 자세 보정각에 대해 유도하였으며, 동체 방향(Heading)각의 경우 60sec를 지난 후 1°이내의 변동률로 안정되는 것을 알 수 있었다. 이를 바탕으로 개할지와 준개할지로 구분하여 각 시스템 단독으로 동적 위치결정을 실험한 결과 개할지의 DGPS 단독 시스템인 경우 정확도 면에서는 우수하였지만 데이터 취득이 미비하여 이동간 거리가 12m 내외임을 알 수 있었으며, DGPS/IMU 결합 시스템의 경우 정확도와 데이터 취득 및 이동간 거리가 0.3m 내외임을 알 수 있었다. 준개할지에서 DGPS 단독 시스템의 경우 데이터 취득이 불가능한 곳을 제외하고 평균과 표준 오차를 구한 결과 DGPS〈 FIMU〈 DGPS/IMU 순으로 정확도가 우수한 것을 알 수 있었으며 이동간 거리는 개할지와 마찬가지였다. 그리고 DGPS의 경우 데이터 취득이 불가능한 곳을 여러 구간으로 비교하였을 때 DGPS 단독 시스템의 경우 최대 41.5m 가량 궤적에서 벗어나지만 결합 시스템의 경우 최대 2.2m 이내에 궤적을 구할 수 있었으며, 평균과 표준 오차를 크게 향상시킬 수 있었다. 이러한 항법 시스템을 결합하여 측량분야에 응용해 수치도화 작업내규의 지도에서 위치오차 0.2mm 오차와 비교하였을 때 축척 1 : 1,000 수치지도 작업까지도 가능한 것을 알 수 있었다.

• 한국지구과학회지
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• 제40권2호
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• pp.119-134
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• 2019

기상청 일사관측소 관측환경 분석을 위하여 수치표고모델(DEM)과 태양복사모델을 이용하여 주변지형에 의한 차폐와 하늘시계요소(SVF) 및 일사량을 산출하였다. 지형고도자료(10 m 해상도)를 통해 관측소를 중심으로 주변 25 km내의 지형들을 이용하여 스카이라인과 SVF를 계산하였다. 또한, 일사관측소별 산출된 천기도와 스카이라인을 중첩하여 지형에 의한 차폐를 분석하였다. 특히 인천 관측소는 주변지형의 차폐가 적었고 청송군과 추풍령 관측소는 주변 지형에 의한 차폐가 큰 관측소로 나타났다. 태양복사모델을 이용하여 동일 조건에서 지형 특성에 따른 일사량을 산출하여 지형에 의한 기여도를 분석하였다. 연누적 일사량 계산결과, 청송군 관측소의 경우 수평면 일사량과 비교하였을 때 직달일사량은 12.0% 이상 차폐되었고 산란일사량은 5.6% 그리고 전천일사량은 4.7% 감소하였다. 평균 일누적 일사량을 기준으로 편차를 분석하였을 때 0.3% 이상 전천일사량이 감소되는 지점은 6개 관측소였다. 42개 관측소 중 8소는 관측소의 이전 또는 관측장비의 이동설치가 시급한 것으로 분석되었고 1/2 이상(24소)의 관측소는 일사관측환경에 대한 검토가 필요한 것으로 분석되었다. DEM자료는 관측소 주변의 인공구조물과 식생 등이 포함되지 않기 때문에 더 상세한 관측환경분석이 요구된다.

• Asian Journal of Atmospheric Environment
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• 제7권1호
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• pp.25-37
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• 2013

Open biomass burning (excluding biofuels) is an important contributor to air pollution in the Asian region. Estimation of emissions from fires, however, has been problematic, primarily because of uncertainty in the size and location of sources and in their temporal and spatial variability. Hence, more comprehensive tools to estimate wildfire emissions and that can characterize their temporal and spatial variability are needed. Furthermore, an emission processing system that can generate speciated, gridded, and temporally allocated emissions is needed to support air-quality modeling studies over Asia. For these reasons, a biomass-burning emissions modeling system based on satellite imagery was developed to better account for the spatial and temporal distributions of emissions. The BlueSky Framework, which was developed by the USDA Forest Service and US EPA, was used to develop the Asian biomass-burning emissions modeling system. The sub-models used for this study were the Fuel Characteristic Classification System (FCCS), CONSUME, and the Emissions Production Model (EPM). Our domain covers not only Asia but also Siberia and part of central Asia to assess the large boreal fires in the region. The MODIS fire products and vegetation map were used in this study. Using the developed modeling system, biomass-burning emissions were estimated during April and July 2008, and the results were compared with previous studies. Our results show good to fair agreement with those of GFEDv3 for most regions, ranging from 9.7 % in East Asia to 52% in Siberia. The SMOKE modeling system was combined with this system to generate three-dimensional model-ready emissions employing the fire-plume rise algorithm. This study suggests a practicable and maintainable methodology for supporting Asian air-quality modeling studies and to help understand the impact of air-pollutant emissions on Asian air quality.