• 한국수자원학회논문집
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• 제57권5호
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• pp.333-346
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• 2024

수량과 수질 및 수생태를 동시에 고려한 수자원 관리를 위해서는 신뢰도 높은 중기 유량 예측 기술이 필수적이다. 이를 위해서는 기상자료의 특성에 대한 이해와 더불어, 시공간 해상도가 낮은 기상예측 정보를 고해상도 분포형 수문모형에서 효과적으로 활용하는 기술이 중요하다. 본 연구에서는 분포형 수문모형 WRF-Hydro와 선행시간 288시간까지의 기상정보를 제공하는 Global Data Assimilation and Prediction System (GDAPS)를 활용해 고해상도 중기 유량 예측을 수행하고 적용성을 검토하였다. 이를 위해 대상 유역인 낙동강 지류 금호강 유역에 대해 100 m 공간해상도의 WRF-Hydro모형을 구축하고 기상지상관측자료 Automatic Weather Stations (AWS)& Automated Synoptic Observing Systems (ASOS), 기상수치예보모형 GDAPS, 기상재분석자료 Global Land Data Assimilation System (GLDAS)를 입력자료로 적용한 유량 예측 모의 결과를 비교하였다. 2020~2022년 기간 3개의 강우사상에 대해 유역 평균 누적 강우량을 분석 결과, AWS&ASOS대비 GDAPS는 36%~234%, GLDAS 재분석자료는 80%~153% 범위의 과소 및 과대 산정되었음을 확인하였다. AWS&ASOS입력자료로 한 유량 예측 결과는 KGE, NSE지표가 유역 말단 강창교 지점 기준 0.6이상이었으나, GDAPS 기반 유량 모의는 강우 사상에 따라 KGE 값이 0.871~-0.131로 큰 변동성이 확인되었다. 한편, 첨두 유량 오차는 GDAPS가 GLDAS보다 크거나 비슷했지만, 첨두 홍수 발생시간의 오차는 AWS&ASOS, GDAPS, GLDAS가 각각 평균 3.7시간, 8.4시간, 70.1시간으로, 첨두 발생시간 측면에서는 GDAPS의 오차가 GLDAS보다 적었다. GDAPS를 입력자료로 한 WRF-Hydro 고해상도 중기 유량 예측은 첨두 유량의 불확실성은 크지만, 첨두 유량 발생시점에 대한 정확도는 상대적으로 높아 수자원 시설 운영에 효과적으로 활용될 수 있을 것으로 판단된다.

• Ocean and Polar Research
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• 제42권1호
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• pp.49-61
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• 2020

We analyzed the morphological characteristics of OCC (Ocean Core Complexes) in the middle part of the Central Indian Ridge (MCIR) using high-resolution geophysical data recorded on the Deep-Tow SideScan Sonar IMI-30 system. In terms of slope-gradient variations calculated from the high-resolution bathymetry data, the normal faults formed by seafloor spreading were associated generally with slopes > 30° and resulted in high backscatter intensities, which reflect more topographic effects than acoustic medium variation. However, the areas associated with gentle slopes < 10° tend to show the backscatter intensities reflecting the acoustic characteristic of the medium. We show that the detachment faults exposing the OCCs were initiated with high-angle normal faults (58°) exhibiting outward and inward dips of a breakaway zone. In order to examine the spatial distribution of OCC structures, we characterized the transition from magmatic-dominant seafloor with abyssal hills to tectonic-dominant seafloor with OCC using the down-slope direction variation. The slope direction of the seafloor generally tends to be perpendicular to the ridge azimuth in the magmatic-dominant zone, whereas it becomes parallel to the given ridge azimuth near the OCC structures. Therefore, this spatial change of seafloor slope directions indicates that the formation of OCC structures is causally associated with the tectonic-dominant spreading rather than magmatic extension. These results also suggest that the topographical characteristics of seafloor spreading and OCC structures can be distinguished using high-resolution geophysical data. Thus, we propose that the high-resolution bathymetry and backscatter intensity data can help select potential areas of exploitation of hydrothermal deposits in MCIR effectively.

• 한국컴퓨터그래픽스학회논문지
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• 제13권4호
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• pp.7-12
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• 2007

최근들어 디지털 영상 기술의 발달로 많은 영화들이 디지털화되어 제작되고 있고, 이러한 디지털 영화를 직접 상영할 수 있는 디지털 시네마로의 전환이 빠르게 진행되고 있다. 하지만 아직 까지 디지털시네마에서 요구하는 2K이상의 고해상도를 지원하는 촬영 장비는 매우 고가이기 때문에 디지털 영화의 제작에 걸림돌이 되고 있다. 본 논문에서는 이러한 문제를 저가의 일반 비디오 카메라와 디지털 스틸 카메라의 조합을 통해 해결할 수 있는 방법을 제시한다. 즉, 비디오 카메라로 촬영한 저해상도 비디오 영상과 동시에 일정한 간격의 키프레임마다 함께 촬영된 고해상도 이미지들을 이용하여 새로운 고해상도 비디오 영상을 합성하는 것이다. 비디오 합성은 프레임 단위로 이루어지는데, 먼저 현재 프레임의 픽셀마다 대응되는 점의 위치를 앞뒤 키프레임들에서 찾는다. 대응점은 현재 프레임과 키프레임 간의 광흐름(optical flow)을 계산하여 찾게 된다. 대응점이 구해지면 키프레임의 고해상도 이미지에서 대응점 위치의 이미지 블럭을 가져와 현재 프레임의 해당 픽셀 위치에 복사한다. 만일 키프레임에서의 대응점을 찾을 수 없는 경우에는 현재 저해상도 비디오 프레임의 확대 이미지를 빈곳 채움에 이용하여 이미지를 완성한다. 본 연구의 결과는 고해상도 비디오 합성 외에 비사실적 비디오 렌더링 등과 같은 영상 효과의 구현에도 적용할 수 있다.

• Mass Spectrometry Letters
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• 제2권1호
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• pp.1-7
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• 2011

China's rapid economic growth has resulted in significant environmental side effects. Therefore, China has been interested in reducing her dependence on foreign oil and gas by developing technologies needed for hydrogen, in addition to her increasing energy mix of nuclear and renewable energy form, such as solar and wind power. There are three isotopes of hydrogen, i.e. protium (P or H), deuterium (D), and tritium (T). Both deuterium and tritium are important materials in nuclear fuel cycle industry. Tritium is one of the critical radioactive nuclides. Planning for and implementing contamination control as a part of normal operation and maintenance activities is an important function in any hydrogen facility, especially tritium facility. The development of hydrogen isotopes analysis is the key issues in this area. Mass spectrometry (MS) with medium (about 600) and high resolution (> 1,400) is commercially available; however, the routine analysis of hydrogen isotopes is done with low-resolution MS (< 200) in China. This paper summarizes the progress of MS measurement technology for hydrogen isotope abundance in China, focusing on our lab's research program and technical status. An analyzing method has been introduced for accurate measurement of tritium abundance in the H.D.T system by low resolution MAT-253 MS. The quotient of compression ratio coefficient is determined by building up equipment for laboratory-scale preparation of secondary standard gases and by considering the difference in sensitivity between hydrogen isotopes. The results show that the measured value is reproducible within the relative error range of 0.8% for gas samples of different tritium abundance.

• 천문학회보
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• 제37권1호
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• pp.79.2-79.2
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• 2012

This study is aim to understand the distribution and the property of LISM (local interstellar medium) using the high resolution spectra of the 26 early type stars in the five open clusters ( IC 4665, Stephenson 1, Collinder 359, Roslund 5 and Collinder 70). These spectra have been observed by BOES in Bohyunsan observatory from 2009 November to 2011 Feburary, of which resolution is 45,000. We used IRAF for the data reduction (Bias subtraction, Flat-field division, and wavelength calibration) and DECH for the deriving the equivalent widths of 4 interstellar lines - Ca II K (3934${\AA}$), Na I D (5890, 5896${\AA}$) and K I (7698${\AA}$) and the column densities of those elements in LISM toward the clusters. The results of this study provide clues for better understanding of the LISM toward these clusters.

• 천문학회지
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• 제40권4호
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• pp.131-132
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• 2007

The research of OH maser emission sources with high angular resolution is complicated by the effects of interstellar scattering: more over, most of the OH maser sources are located in the galactic plane where the scattering is largest. However, the data available from pulsar studies on the spatial distribution of the amount of scattering indicate that there is a strong non-uniformity in the distribution of the amount of scattering material. There are directions in the galactic plane where the scattering is an order of magnitude higher than the average, as well as directions where the scattering is much lower. The latter provide an opportunity to investigate OH masers with the full angular resolution offered by very long baseline interferometry instruments, like the VLBA, and measure their true angular size, shape and brightness temperature. We have observed approximately 100 OH maser sources, distributed all over the northern hemisphere, with the VLBA in order to study the scattering properties of the interstellar medium.

• 대한자원환경지질학회:학술대회논문집
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• 대한자원환경지질학회 2005년도 춘계 학술발표회 논문집
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• pp.148-151
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• 2005

Field-scale DNAPL dissolution is controlled by the topology of DNAPL distributions with respect to the velocity field. A high resolution percolation model was developed and employed to simulate the distribution of DNAPL within source zones. Statistically anisotropic permeability values and capillary parameters were generated for 10${\times}$10${\times}$10 m domains at a resolution of 0.05 to 0.1 m for various statistical properties. TCE leakage was simulated at various rates and the distribution of residual DNAPL in 'fingers' and 'lenses' was computed. Variations in finger and lens geometries, frequencies, average DNAPL saturations, and overall source topology were predicted to be strongly influenced by statistical properties of the medium as well as by injection rate and fluid properties. Model results were found to be consistent with observations from controlled DNAPL release experiments reported in the literature. The computed distributions of aquifer properties and DNAPL were utilized to perform high-resolution numerical simulations of groundwater flow and dissolved transport. Simulations were performed to assess the effect of grout or foam injection in bore holes within the source zone and of shallow point-releases of fluids with various properties on dissolution in DNAPL dissolution rate, even for widely spaced injection points. The results indicate that measures that induced partial flow reductions through DNAPL source zones can significantly decrease dissolution rates from residual DNAPL. The benefit from induced partial flow reductions is two-fold: 1) local flow reduction in DNAPL contaminated zones reduces mass transfer rates, and 2) contaminant flux reductions occur due to the decrease in groundwater velocity

• Journal of Communications and Networks
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• 제17권3호
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• pp.275-285
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• 2015

To improve the efficiency of carrier sense multiple access (CSMA)-based medium access control (MAC) protocols, CSMA with collision resolution (CSMA/CR) has been proposed. In the CSMA/CR, a transmitting station can detect a collision by employing additional sensing after the start of a data transmission and then resolve the next collision that might occur by broadcasting a jam signal during a collision detection (CD) period. In this paper, we analyze the delay of a CSMA/CR based on a generic p- persistent CSMA model and obtain the minimum achievable delay of the CSMA/CR by finding the optimal length of the CD period according to the number of contending stations. Through this delay analysis, we also investigate the throughput-delay characteristics of the CSMA/CR protocol according to various parameters. Analysis and simulation results show that the CSMA/CR has a considerably lower delay and its throughput-delay characteristic is significantly improved than the conventional CSMA/CA and wireless CSMA/CD protocols.

• 천문학회보
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• 제40권1호
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• pp.41.4-42
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• 2015

The Immersion Grating Infrared Spectrograph (IGRINS) is the first of a new generation of infrared instruments with high sensitivity, high spectral resolution, and broad spectral grasp. IGRINS, a joint project of the University of Texas and the Korea Astronomy and Space Science Institute, designed and constructed by a team at UT, KASI, and Kyung Hee University, has been available to the Korean and Texas communities on the McDonald Observatory 2.7m telescope since 2014 September. On this modest-sized telescope, the instrument has 30 times the spectral grasp of CRIRES at the 8m VLT and is only slightly less sensitive. Already, Korean and UT astronomers have produced a raft of new results in star formation studies, investigations of the interstellar medium, and the nature of cool stars. Several programs are under way to detect and study the atmospheres of exoplanets. We will present highlights from the first 6 months of IGRINS operations and look at the future of IR spectroscopy both with IGRINS and with GMTNIRS, a UT/KASI/KHU instrument for the Giant Magellan Telescope.

• Nuclear Engineering and Technology
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• 제49권7호
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• pp.1489-1494
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• 2017

The use of a room-temperature gamma spectrometer is an issue in environmental radiation monitoring. To monitor radionuclides released around a nuclear power plant, suitable instruments giving fast and reliable information are required. High-pressure xenon (HPXe) chambers have range of resolution and efficiency equivalent to those of other medium resolution detectors such as those using NaI(Tl), CdZnTe, and $LaBr_3:Ce$. An HPXe chamber could be a cost-effective alternative, assuming temperature stability and reliability. The CEA LIST actively studied and developed HPXe-based technology applied for environmental monitoring. Xenon purification and conditioning was performed. The design of a 4-L HPXe detector was performed to minimize the detector capacitance and the required power supply. Simulations were done with the MCNPX2.7 particle transport code to estimate the intrinsic efficiency of the HPXe detector. A behavioral study dealing with ballistic deficits and electronic noise will be utilized to provide perspective for further analysis.