• 한국환경과학회지
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• 제14권7호
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• pp.657-667
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• 2005

In this study, we focused on the improvements in the simulation of sea surface wind over the complex coastal area. MM5 model being currently used to predict sea surface wind at Korea Meteorological Administration, was used to verify the accuracy to estimate the local wind field. A case study was performed on clear days with weak wind speed(4 m/s), chosen by the analysis of observations. The model simulations were conducted in the southeastern area of Korea during the selected periods, and observational data such as AWS, buoy and QuikSCAT were used to compare with the calculated wind components to investigate if simulated wind field could follow the tendency of the real atmospheric wind field. Results showed that current operational model, MM5, does not estimate accurately sea surface wind and the wind over the coastal area. The calculated wind speed was overestimated along the complex coastal regions but it was underestimated in islands and over the sea. The calculated diurnal changes of wind direction could not follow well the tendency of the observed wind, especially at nighttime. In order to exceed the limitations, data assimilation with high resolution data and more specificated geographical information is expected as a next best policy to estimate accurately the environment of local marine wind field.

• 한국정보통신학회논문지
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• 제13권9호
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• pp.1973-1979
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• 2009

본 논문에서는 과학영재의 관찰평가를 비교 분석하여 수학 및 과학분야의 영재 학습자와 정보과학영재의 특성을 밝혀내어 정보과학영재의 선발 및 교육에 시사점을 찾으려고 하였다. 연구의 대상은 대학부설과학영재교육원의 기초과정 학습자들로써 분야는 물리, 지구과학, 수학, 정보과학 학습자들이다. 연구의 방법으로는 학습자들의 1년간의 관찰평가를 일원분산분석을 통하여 각 분야별 학습자의 특성을 비교하였다. 그 결과 정보과학영재 학습자는 물리 및 지구과학분야 학습자와 태도 영역과 문제 해결 영역의 세부 영역에서 대부분 다른 특성을 보였으며, 정보 과학 학습자의 과목별 분석에서는 과학보다는 수학과 정보 과목에서 태도 영역의 평가가 비교적 우수하게 분석되었다. 이에 본 연구자는 정보과학영재의 특성이 분명히 존재하며 과학 및 수학 영재 학습자와의 차이는 학습자간의 수준의 문제와 분야별 특성에 기인한 것이라 판단하였다. 본 연구의 결과를 바탕으로 정보과학영재의 선발 및 교육에 적용할 수 있으리라 기대한다.

• 한국지반환경공학회 논문집
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• 제13권12호
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• pp.35-42
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• 2012

연약지반에 구조물을 설치하거나 도로 또는 단지를 조성하는 경우 지지력 부족으로 인한 지반 전단파괴 및 과도한 압밀침하 등 공학적 문제가 발생하게 되어, 강도증가 및 침하억제를 위한 지반 개량공사를 필수적으로 시행하여야 한다. 연약지반을 개량함에 있어 현장계측자료를 바탕으로 한 장기침하량 예측은 선행재하 성토고 및 압밀완료시점 예측을 위한 매우 중요한 요소로 이에 관한 연구가 국내 외 여러 학자들에 의해 진행되고 있다. 본 연구에서는 선행재하 및 연직배수 공법을 적용하여 점성토 연약지반개량을 시행한 연구 대상 지역의 압밀침하 특성을 분석하였으며, 쌍곡선법, ${\sqrt{S}}$법, Asaoka법을 적용하여 압밀도에 따른 예측 침하량과 실측 최종침하량을 비교 분석하여 김포한강지구의 토질특성에 맞는 침하예측기법을 연구하였다. 연구결과에 의하면 3가지 예측방법으로 추정한 침하량과 계측침하량의 오차가 최대 ${\pm}4$% 이내로 실 침하량과 거의 일치하였으며, 예측의 정확도는 Asaoka법, 쌍곡선법, ${\sqrt{s}}$법 순으로 나타났다.

• 천문학회지
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• 제37권5호
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• pp.427-431
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• 2004

We use simulations of large-scale structure formation to study the build-up of magnetic fields (MFs) in the intergalactic medium. Our basic assumption is that cosmological MFs grow in a magnetohy-drodynamical (MHD) amplification process driven by structure formation out of a magnetic seed field present at high redshift. This approach is motivated by previous simulations of the MFs in galaxy clusters which, under the same hypothesis that we adopt here, succeeded in reproducing Faraday rotation measurements (RMs) in clusters of galaxies. Our ACDM initial conditions for the dark matter density fluctuations have been statistically constrained by the observed large-scale density field within a sphere of 110 Mpc around the Milky Way, based on the IRAS 1.2-Jy all-sky redshift survey. As a result, the positions and masses of prominent galaxy clusters in our simulation coincide closely with their real counterparts in the Local Universe. We find excellent agreement between RMs of our simulated galaxy clusters and observational data. The improved numerical resolution of our simulations compared to previous work also allows us to study the MF in large-scale filaments, sheets and voids. By tracing the propagation of ultra high energy (UHE) protons in the simulated MF we construct full-sky maps of expected deflection angles of protons with arrival energies $E = 10^{20}\;eV$ and $4 {\times} 10^{19}\;eV$, respectively. Accounting only for the structures within 110 Mpc, we find that strong deflections are only produced if UHE protons cross galaxy clusters. The total area on the sky covered by these structures is however very small. Over still larger distances, multiple crossings of sheets and filaments may give rise to noticeable deflections over a significant fraction of the sky; the exact amount and angular distribution depends on the model adopted for the magnetic seed field. Based on our results we argue that over a large fraction of the sky the deflections are likely to remain smaller than the present experimental angular sensitivity. Therefore, we conclude that forthcoming air shower experiments should be able to locate sources of UHE protons and shed more light on the nature of cosmological MFs.

• 대기
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• 제28권2호
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• pp.163-174
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• 2018

In order to assimilate MHS satellite data into the convective scale model at KMA, ATOVS data are reprocessed to utilize the original high-resolution data. And then to improve the preprocessing experiments for cloud detection were performed and optimized to convective-scale model. The experiment which is land scattering index technique added to Observational Processing System to remove contaminated data showed the best result. The analysis fields with assimilation of MHS are verified against with ECMWF analysis fields and fit to other observations including Sonde, which shows improved results on relative humidity fields at sensitive level (850-300 hPa). As the relative humidity of upper troposphere increases, the bias and RMSE of geopotential height are decreased. This improved initial field has a very positive effect on the forecast performance of the model. According to improvement of model field, the Equitable Threat Score (ETS) of precipitation prediction of $1{\sim}20mm\;hr^{-1}$ was increased and this impact was maintained for 27 hours during experiment periods.

• 천문학회보
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• 제45권1호
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• pp.46.2-46.2
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• 2020

Dust ejection activities have been discovered from a few tens of asteroids since the first confirmation in 2006. Those objects are known as active asteroids. They provide good observational chances to study ongoing phenomena in the solar system such as sublimation of icy volatiles, mutual collisions among asteroids, rotational disintegrations, thermal fatigue, etc. Although dust ejection mechanisms of individual cases have been investigated through observations, the frequencies of the events and their connection to the overall evolutionary budget of the solar system have not yet been studied thoroughly, mainly because previous studies were based on serendipitous discoveries without any systematic surveys of these objects. In this work, we made wide-field monitoring observations of asteroids using Korea Microlensing Telescope Network (KMTNet) during the 2018/2019 winter season. Among 3,644 asteroids in the field-of-view, we detected nine candidates of brightness enhancements which we suspect as possible activities. It is still possible that some of those brightness increases have caused by long-term rotations. However, our observed frequency and brightness enhancements size-frequency distribution agrees with the expectations from impacts with decimeter sized objects, when the main belt objects size-frequency distribution observed down to decameter sized bodies are extrapolated to decimeter size.

• 한국환경과학회지
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• 제14권3호
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• pp.297-309
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• 2005

Recently air quality modeling studies for industrial complex and large cities located in the coastal regions have been carried out Especially, the representation of atmospheric flow fields within a model domain is very important, because an adequate air quality simulation requires an accurate portrayal of the realistic three­dimensional wind fields. Therefore this study investigated effect of using high resolution terrain height data and FDDA with observational data to reflect local characteristics in numerical simulation. So the experiments were designed according to FDDA and the detail terrain height with 3sec resolution or not Case 30s was the experiment using the terrain height data of USGS without FDDA and Case 3s was the experiment using the detail terrain height data of Ministry of Environment without FDDA and Case 3sF was experiment using the detail terrain height data of Ministry of Environment with FDDA. The results of experiments were more remarkable, In Case 3s and Case 3sF, temperature indicated similar tendency comparing to observational data predicting maximum temperature during the daytime and wind speed made weakly for difference of terrain height Also Case 3sF had more adequate tendency than Case 3s at dawn.

• 한국콘텐츠학회논문지
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• 제16권7호
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• pp.513-521
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• 2016

본 연구는 간호대학생의 분만실 실습 중 수행내용을 파악하고 임상실습 환경에 따른 간호대학생의 실습 수행도 및 만족도를 분석하여 실습의 질 향상을 위한 개선방안을 제시하고자 하였다. 연구결과 간호대학생의 분만실 임상실습은 대부분 관찰 위주로 진행되고 있었고, 제한된 영역에서만 직접수행과 보조적 수행을 경험하였다. 간호대학생의 임상수행 만족도는 69%정도의 비교적 낮은 수준을 보였다. 임상실습지에 따른 차이를 분석한 결과 여성전문병원의 분만실에서 실습 한 간호대학생은 종합병원에서 보다 더 많은 관찰을 수행 할 수 있었고, 그에 따라 만족도 점수 또한 높았다. 분만실 임상실습에서 관찰 및 보조적 수행이 많을수록 만족도는 상승하였다. 결과에서 확인된 실습 중 부족한 직접수행은 시뮬레이션기반 임상실습 등을 통해 보완할 수 있을 것이다. 또한 병원 실무자와의 긴밀한 의사소통을 기반으로 실습지를 확보하고, 다양한 간호대상자를 경험하고 관찰할 수 있도록 지도하는 것은 간호대학생의 임상실습 만족도와 질 향상을 위한 전략으로서 제시될 수 있겠다.

• 융합신호처리학회논문지
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• 제18권1호
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• pp.13-20
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• 2017

본 논문에서는 KVN의 광대역 VLBI 관측을 위한 백엔드 시스템으로써 도입한 32 Gbps 급 관측장비의 기본적인 시험결과에 대해 고찰한다. 천문학자들은 천체의 초미세 구조를 관측하고자 성능이 우수한 큰 전파망원경을 만들고 싶지만, 많은 돈이 소요된다. 따라서 민감도를 높이기 위해 수신시스템의 성능개선이나 넓은 주파수 대역폭을 관측하는 방법을 도입하고 있다. 이를 위해 본 연구에서는 넓은 관측 주파수 대역폭을 관측하기 위해서는 아날로그 신호를 초고속으로 변환하는 광대역 샘플링 방법과 디지털 필터링을 수행하는 광대역 샘플러를 도입하였다. 광대역 샘플러(OCTAD-K)는 최대 16Gsps-2bit 샘플링을 지원하며, 디지털필터링 기술을 이용하여 다양한 관측대역폭의 관측을 지원한다. 특히 KVN의 4주파수 동시관측시스템과 VERA의 2-beam 관측시스템을 지원할 수 있도록 설계되었다. 그리고 편파관측도 지원할 수 있으며, 관측데이터의 출력의 표준 VDIF 형식을 지원한다. 본 논문에서는 광대역 샘플러를 도입하기 전 수행한 공장검수와 현장시험을 수행한 후 시스템의 성능결과와 문제점 해결 등에 대해 자세히 기술한다.

• 천문학회보
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• 제36권1호
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• pp.36.1-36.1
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• 2011

It is generally believed that eruptive phenomena in the solar atmosphere such as solar flares and coronal mass ejections (CMEs) occur in the solar active regions with complex magnetic structures. Magnetic helicity has been recognized as a useful parameter to measure the complexity such as twists, kinks, and inter-linkages of magnetic field lines. The objective of this study is to understand a long-term (a few days) variation of magnetic helicity in active regions and its relationship with the energy buildup and instability leading to flares and CMEs. Statistical studies of flare productivity and magnetic helicity injection in about 400 active regions were carried out. The temporal variation of magnetic helicity injected through the photosphere of active regions was also examined related to 46 CMEs. The main findings in this study are as follows: (1) the study of magnetic helicity for active regions producing major flares and CMEs indicates that there is always a significant helicity injection through the active-region photosphere over a long period of 0.5 - a few days before the flares and CMEs; (2) for the 30 CMEs under investigation, it is found that there is a fairly good correlation (linear correlation coefficient of 0.71) between the average helicity injection in the CME-productive active regions and the CME speed. Beside the scientific contribution, a major impact of this study is the observational discovery of a characteristic variation pattern of magnetic helicity injection in flare/CME-productive active regions which can be used for the improvement of solar eruption forecasting.