• 한국해양공학회지
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• 제19권1호
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• pp.14-19
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• 2005

As a basic study for establishing the input conditions of a forecasting/estimating model, used for deep-sea water drainage to the ocean, this study was carried out as follows: 1) estimating the amount of river discharge and pollutant loads into the developing region of deep sea water in the East Sea, Korea, 2) a field observation of tidal current, vertical water temperature, and salinity distribution, 3) 3-D numerical experiment of tidal current to analyze the physical oceanographic status. The amount of river discharge flowing into this study area was estimated at about $462.7{\times}103 m\^3/day$ of daily mean in 2002. Annual mean pollutant load of COD, TN, and TP were estimated at 7.02 ton-COD/day, 4.06 ton-TN/day, and 0.39 ton/day, respectively. Field observation of tidal current normally shows 20-40cm/sec of current velocity at the surface layer, and it decreases under 20cm/sec as the water depth increases. We also found a stratification condition at around 30m water depth in the observation area. The differences in water temperature and salinity, between the surface layer and the bottom layer, were about 18 C and 0.8 psu, respectively. On the other hand, we found a definite trend of 34 psu salinity water mass in the deep sea region.

• 대기
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• 제17권4호
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• pp.435-453
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• 2007

KEOP (Korea Enhanced Observing Period)-2004 intensive summer observation was carried out from 20 June to 5 July 2004 over the Southwestern part of the Korean peninsula. In this study, the effects of KEOP-2004 intensive observation data on the simulation of precipitation system are investigated using KLAPS (Korea Local Analysis and Prediction System) and PSU/NCAR MM5. Three precipitation cases during the intensive observation are selected for detailed analysis. In addition to the control experiments using the traditional data for its initial and boundary conditions, two sensitivity experiments using KEOP data with and without Jindo radar are performed. Although it is hard to find a clear and consistent improvement in the verification score (threat score), it is found that the KEOP data play a role in improving the position and intensity of the simulated precipitation system. The experiments started at 00 and 12 UTC show more positive effect than those of 06 and 18 UTC. The effect of Jindo radar is dependent on the case. It plays a significant role in the heavy rain cases related to a mesoscale low over Changma front and the landing of a Typhoon. KEOP data produce more strong difference in the 06/18 UTC experiments than in 00/12 UTC, but give more positive effects in 00/12 UTC experiments. One of the possible explanations for this is that : KEOP data could properly correct the atmosphere around them when there are certain amounts of data, while gives excessive effect to the atmospheric field when there are few data. CRA analysis supports this reasoning. According to the CRA (Contiguous Rain Area) analysis, KEOP data in 00/12 UTC experiments improve only the surrounding area, resulting in essentially same precipitation system so the effects remain only in each convective cell rather than the system itself. On the other hand, KEOP data modify the precipitation system itself in 06/18 UTC experiments. Therefore the effects become amplified with time integration.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2007년도 Proceedings of ISRS 2007
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• pp.397-400
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• 2007

For mapping the distribution of heavy metals in the mining area, field spectroscopy and hyperspectral remote sensing were used in this study. Although heavy metals are spectrally featureless from the visible to the short wave infrared range, possible variations in spectral signal due to heavy metals bound onto minerals can be explained with the metal binding reaction onto the mineral surface. Variations in the spectral absorption shapes of lattice OH and oxygen on the mineral surface due to the combination of heavy metals were surveyed over the range from 420 to 2400 nm. Spectral parameters such as peak ratio and peak area were derived and statistically linked to metal concentration levels in the streambed samples collected from the dry stream channels. The spatial relationships between spectral parameters and concentrations of heavy metals were yielded as well. Based on the observation at a ground level for the relationship between spectral signal and metal concentration levels, the spectral parameters were classified in a hyperspectral image and the spatial distribution patterns of classified pixels were compared with the product of analysis at the ground level. The degree of similarity between ground dataset and image dataset was statistically validated. These techniques are expected to support assessment of dispersion of heavy metal contamination and decision on optimal sampling point.

• 한국수자원학회논문집
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• 제40권11호
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• pp.841-849
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• 2007

본 연구에서는 우량계와 강우 레이더를 함께 이용하는 경우의 통합관측 효과를 검토하였다. 통합관측효과는 서로 직교하는 관측방법의 결합에 따른 관측오차의 감소를 고려함으로써 평가된다. 구체적인 적용 예로서 금강유역에 대하여 강우 레이더가 추가로 설치되는 경우 우량 관측망 밀도를 어느 정도까지 조정할 수 있는지에 대한 평가를 수행하였다. 이를 위해 North and Nakamoto(1989), Yoo et al. (1996), 유철상(1997)의 관측오차 관련 연구를 응용하였으며, 강우장의 모형화를 위해서는 그 구조가 간단한 NFD 모형을 이용하였다. 모형의 매개변수는 금강유역의 28개 우량 관측소 시자료를 이용하여 추정된 강우장의 특성치(상관거리 및 상관시간)를 이용하여 결정하였고, 레이더의 운영 특성은 임의로 가정하였다. 본 연구에서는 WMO(1994)의 추천 우량관측 밀도와 금강유역에 설치된 우량 관측 밀도를 고려하여 레이더의 도입으로 인한 우량 관측 밀도의 조정 방안을 제시하였다.

• 한국지구과학회지
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• 제43권1호
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• pp.1-22
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• 2022

운장산 천문대에 있는 원격 유성 분광 관측 시스템의 설치 및 운영에 대해 자세히 설명한다. 총 3대의 고감도 CCD 카메라가 설치되었으며 2대의 CCD 카메라에는 렌즈 전면에 회절 격자를 부착하였다. 시스템은 2019년 11월에 설치되었고, f/1.2 렌즈와 결합된 고감도의 "Watec-902H2" 카메라가 사용되었다. 스펙트럼 관찰을 위한 회절 격자는 500 l/mm이 사용되었다. 관측은 2019년 11월부터 2020년 6월까지 진행되었다. 유성 탐지 및 후속 분석을 위해 SonotaCo UFO 소프트웨어 제품군을 사용했으며, 유성 스펙트럼을 분석하기 위해서는 RSpec 소프트웨어를 사용하였다. 관측영상을 활용하기 위해 Astronomical Calibration과 Photometric Calibration을 수행하였고, 최종적으로 유성의 화학 성분을 분석하였다. 우리는 유성 분광 관측 시스템의 설치와 설정/운영 경험을 설명하고 첫 번째 관측 결과를 제시한다. 또한 결과를 통해 유성의 기원에 대한 간략한 정보를 제공하고자 한다.

• Advances in aircraft and spacecraft science
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• 제9권5호
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• pp.449-462
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• 2022

Space-telescopes placed in the Sun-Earth second Lagrange point (L2) observe the sky following a scan strategy that is usually based on a spin-precession motion. Knowing which regions of the sky will be more observed by the instrument is important for the science operations and the instrument calibration. Computing sky observation parameters numerically (discretizing time and the sky) can consume large amounts of time and computational resources, especially when high resolution isrequired.This problem becomesmore critical if quantities are evaluated at detector level instead of considering the instrument entire Field of View (FoV). In previous studies, the authors have derived analytic solutions for quantities that characterize the observation of each point in the sky in terms of observation time according to the scan strategy parameters and the instrument FoV. Analytic solutions allow to obtain results faster than using numerical methods as well as capture detailed characteristics which can be overseen due to discretization limitations. The original approach is based on the analytic expression of the instrument trace over the sky. Such equations are implicit and thusrequiresthe use of numeric solversto compute the quantities.In this work, a new and simpler approach for computing one ofsuch quantities(mean observation time) is presented.The quantity is first computed for pure spin motion and then the effect of the spin axis precession is incorporated under the assumption that the precession motion is slow compared to the spin motion.In this sense, this new approach further simplifies the analytic approach, sparing the use of numeric solvers, which reduces the complexity of the implementation and the computing time.

• 한국지구과학회지
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• 제26권1호
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• pp.41-57
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• 2005

본 연구의 목적은 학생들로 하여금 실제 야외지질조사를 효과적으로 수행하기 위한 교육 자료를 개발하는 것이다. 이를 위하여 시대를 달리하는 다양한 암석과 지질구조를 가지고 있고 지리적으로 접근하기 편리한 음성분지의 남동부 두타산 일대를 대상으로 선정하였다. 음성분지의 야외지질 실습코스에는 13개의 관찰지점이 있으며 실제 현장에서 각 관찰 지점별로 학생들이 활동할 수 있도록 야외학습자료를 제시하였다. 이를 위해 일반 지형도나 수치 지형도를 이용하여 스스로 노선지질도를 작성하도록 하였으며 큰 구조나 서로 다른 암상과의 관계를 광역적으로 알 수 있도록 항공사진을 첨가하였다. 또한 각 관찰 지점마다 노두 및 편광 현미경 사진을 제시하여 야외학습에서 경험할 수 있는 환경으로 설계하여 실제로 야외에서 겪게 되는 갈등 요인을 최소화 할 수 있도록 하였다. 이렇게 구현된 야외지질조사자료는 충북대학교 사범대학 지구과학 수강자를 대상으로 학생들의 태도를 조사하였으며, 그 결과 정의적 측면에서 학생들이 야외학습을 수행하는데 도움이 된다는 긍정적인 변화를 보였으며, 특히 지구과학에 관한 구체적인 개념 형성에 많은 도움이 되는 것으로 분석되었다.

• 한국주조공학회지
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• 제17권1호
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• pp.76-84
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• 1997

An investigation of the effects of transverse magnetic field on melt convection and macrosegregation in vertical Bridgman growth of Te doped InSb was carried out by means of microstructure observation, the measurement of Te distribution by Hall measurement, electrical resistivity measurement and X-ray analysis. Prior to the experiments, interface stability, convective instability and suppression of convection by magnetic field were examined. A thermosolutal convection in the Te doped InSb melt occurred in the examined growth condition without magnetic field. The effective distribution coefficient, $K_{eff}$, was about 0.35 without magnetic field, 0.45 with magnetic field of 2kG, and 0.7 at 4kG. It was found that the stronger the applied magnetic field was, the more the convection was suppressed.

• 한국지구과학회지
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• 제24권1호
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• pp.7-21
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• 2003

The state-of-art third generation wave prediction model WAM was applied to the Korean seas for a winter monsoon period of January 1997. The wind field used in the present study is the global NSCAT-ERS/NCEP blended winds, which was further interpolated using a bi-cubic spline interpolator to fine grid limited area shallow water regime surrounding the Korean seas. To evaluate and investigate the accuracy of WAM, the hindcasted wave heights are compared with observed data from two shallow water buoys off Chil-Bal and Duk-Juk. A detailed study has been carried with the various meteorological parameters in observed buoy data and its inter-dependency on model computed wave fields was also investigated. The RMS error between the observation and model computed wave heights results to 0.489 for Chil-Bal and 0.417 for Duk-Juk. A similar comparison between the observation and interpolated winds off Duk-Juk show RMS error of 2.28 which suggest a good estimate for wave modelling studies.

• 천문학회보
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• 제40권2호
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• pp.44.3-45
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• 2015

The 2007 event occurred at 17P/Holmes is known as the most energetic cometary outburst in the history of modern astronomical observations. At this conference, we report our new observation of the comet one orbital period after the event. We thus made the observation of 17P/Holmes in 2014 September using the Kiso Wide Field Camera (KWFC) attached to the 105 cm Schmidt telescope at the Kiso Observatory. It is known that dust particles are thought to converge on the orbital plane of the parent body at the opposite end of the dust ejection viewed from the Sun. Similar phenomenon occurs when dust particles complete one orbital revolution (what we call, neck-line structures). We succeeded in the detection of the dust ejecta of the 2007 outburst by means of the neck-line. With the image, we plan to discuss the ejection velocity and the total mass of the ejecta to deepen our understanding of the historical event.