• Journal of the Korean Statistical Society
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• 제36권4호
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• pp.543-556
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• 2007

In successive sampling on two occasions the problem of estimating a finite population quantile has been considered. The theory developed aims at providing the optimum estimates by combining (i) three double sampling estimators viz. ratio-type, product-type and regression-type, from the matched portion of the sample and (ii) a simple quantile based on a random sample from the unmatched portion of the sample on the second occasion. The approximate variance formulae of the suggested estimators have been obtained. Optimal matching fraction is discussed. A simulation study is carried out in order to compare the three estimators and direct estimator. It is found that the performance of the regression-type estimator is the best among all the estimators discussed here.

• 천문학논총
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• 제30권2호
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• pp.87-88
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• 2015

We present results of our R-band polarimetry of a bright-rimmed cloud, IC1396A (with BRC 36), associated with the H II region S131 and the cometary globule LDN 1616 to study their magnetic field geometry. The distances of these clouds have been reported to be ~ 750 pc and ~ 450 pc, respectively in the literature. The young open cluster Trumpler 37 in the vicinity of IC1396A and the high mass stars in the Orion belt near L1616 are found to be responsible for the structure of these clouds. We made polarimetry of foreground stars inferred from their distances measured by the Hipparcos satellite to subtract the foreground contribution to the observed polarization results. We discuss the optical polarimetric results and compare our findings with MHD simulations towards BRCs and CGs.

• 조명전기설비학회논문지
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• 제24권1호
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• pp.19-27
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• 2010

천공커버법칙은 기상청에서 제공하는 전운량을 활용하여 천공 상태를 결정할 수 있으며, HCI(Hourly Clearness Index) 방법은 측정된 태양의 수평 일사량을 이용하여 천공 상태를 결정한다. HCI 방법에는 Erbs et al. 방법(1982)과 Orgill and Holland 방법(1977) 등이 있으나, 이와 같은 기존의 방법은 약 30여 년전에 수립된 것으로 현재의 대기 상황과 다소 다르기 때문에 실제 전운량에 의한 천공 상태와 차이를 보인다. 본 연구의 목적은 HCI에 의한 천공 구분 방법을 개선하고자 하는데 있으며, 이에 기상청 데이터를 이용한 천공커버법칙에 의한 천공상태와 측정된 수평 일사량을 이용한 HCI의 천공상태를 비교 분석하여 기존 HCI 방법의 시간별 보정 방법을 제안하였다. 그 결과, 보정된 HCI 방법이 기존의 HCI 방법에 비해 천공별 유사성이 다소 향상되었다.

• KIEAE Journal
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• 제14권2호
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• pp.3-10
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• 2014

Impact by estimation error of hourly horizontal global solar radiation in a weather file on building energy performance was investigated in this study. There are a number of weather parameters in a given weather file, such as dry-bulb, wet-bulb, dew-point temperatures; wind speed and direction; station pressure; and solar radiation. Most of them except for solar radiation can be easily obtained from weather stations located on the sites worldwide. However, most weather stations, also including the ones in South Korea, do not measure solar radiation because the measuring equipment for solar radiation is expensive and difficult to maintain. For this reason, many researchers have studied solar radiation estimation models and suggested to apply them to predict solar radiation for different weather stations in South Korea, where the solar radiation is not measured. However, only a few studies have been conducted to identify the impact caused by estimation errors of various solar radiation models on building energy performance analysis. Therefore, four different weather files using different horizontal global solar radiation data, one using measured global solar radiation, and the other three using estimated global solar radiation models, which are Cloud-cover Radiation Model (CRM), Zhang and Huang Model (ZHM), and Meteorological Radiation Model (MRM) were packed into TRY formatted weather files in this study. These were then used for office building energy simulations to compare their energy consumptions, and the results showed that there were differences in the energy consumptions due to these four different solar radiation data. Additionally, it was found that using hourly solar radiation from the estimation models, which had a similar hourly tendency with the hourly measured solar radiation, was the most important key for precise building energy simulation analysis rather than using the solar models that had the best of the monthly or yearly statistical indices.

• 천문학회보
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• 제42권2호
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• pp.43.3-43.3
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• 2017

NGC 6822 is a dwarf irregular galaxy in the Local Group and it is located in 500 kpc, further than the Large Magellanic Cloud and the Small Magellanic Cloud. Therefore, we can study star-forming processes by local condition in NGC 6822 instead of tidal force of the Galactic gravitational field. Hubble V is the brightest of several H II complexes in this galaxy. We observed Hubble V by using IGRINS attached on the 2.7 m telescope at the McDonald Observatory in Texas, US in May 2016. We performed a spectral mapping of $15^{{\prime}{\prime}}{\times} 7^{{\prime}{\prime}}$area on H and K bands, and detected emission lines of bright $Br{\gamma}\;{\lambda}2.1661{\mu}m$ and weak He I ${\lambda}2.0587{\mu}m$. Molecular hydrogen lines of 1-0S(1) ${\lambda}2.1218{\mu}m$, 2-1 S(1) ${\lambda}2.2477{\mu}m$, and 1-0 S(0) ${\lambda}2.2227{\mu}m$ was also detected. These emission lines show the structure of an ionized core and excited surface of clouds by far-ultraviolet photons, photodissociation region (PDR). We present three-dimensional maps of emission line distributions through multi slit scanning data and compare these results with the previous study. This presentation shows the physical structure of the star-forming regions and we discuss a PDR model and an evolution of Hubble V complex.

• 한국음향학회지
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• 제39권5호
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• pp.454-460
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• 2020

음성인식 기능을 제공하는 인공지능 비서들은 정확도가 뛰어난 클라우드 기반의 음성인식을 통해 동작한다. 클라우드 기반의 음성인식에서 시작 단어 인식은 대기 중인 기기를 활성화하는 데 중요한 역할을 한다. 본 논문에서는 공개 데이터셋인 구글의 Speech Commands 데이터셋을 사용하여 스펙트로그램 및 멜-주파수 캡스트럼 계수 특징을 입력으로 하여 모바일 기기에 대응한 저 연산 시작 단어 검출을 위한 합성곱 신경망의 성능을 비교한다. 본 논문에서 사용한 합성곱 신경망은 다층 퍼셉트론, 일반적인 합성곱 신경망, VGG16, VGG19, ResNet50, ResNet101, ResNet152, MobileNet이며, MobileNet의 성능을 유지하면서 모델 크기를 1/25로 줄인 네트워크도 제안한다.

• 한국환경과학회지
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• 제16권3호
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• pp.261-267
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• 2007

In this study, the Slab Ocean Model (SOM) is coupled with an Atmospheric General Circulation Model (AGCM) which developed in University of Kangnung based on the land surface model of Biosphere-Atmosphere Transfer Scheme (BATS). The purposes of this study are to understand radiative role of clouds considering of the atmospheric feedback, and to compare the Clouds Radiative Forcing (CRF) come from the analyses using the clear-cloud sky method and CGCM. The new CGCM was integrated by using two sets of the clouds with radiative role (EXP-A) and without radiative role (EXP-B). Clouds in this two cases show the negative effect $-26.0\;Wm^{-2}$ of difference of radiation budget at top of atmosphere (TOA). The annual global means radiation budget of this simulation at TOA is larger than the estimations ($-17.0 Wm^{-2}$) came from Earth Radiation Budget Experiment (ERBE). The work showed the surface negative effect with $-18.6 Wm^{-2}$ in the two different simulations of CRF. Otherwise, sensible heat flux in the simulation shows a great contribution with positive forcing of $+24.4 Wm^{-2}$. It is found that cooling effect to the surface temperature due to radiative role of clouds is about $7.5^{\circ}C$. From this study it could make an accurate of the different CRF estimation considering either feedback of EXP-B or not EXP-A under clear-sky and cloud-sky conditions respectively at TOA. This result clearly shows its difference of CRF $-11.1 Wm^{-2}$.

• 한국측량학회지
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• 제39권6호
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• pp.401-408
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• 2021

2021년 보행안전법 개정안이 발의되면서 보행자 안전의 근간이 되는 보행자길에 대한 전수조사의 법제화 및 의무화 가능성이 높아졌다. 이에 본 연구에서는 보급형 드론과 상용프로그램을 사용하여 사진측량 기법으로 가로공간의 포인트 클라우드 데이터를 생성하고 분석하는 적정비용의 조사방법론을 제시하고자 하였다. 또한 전국 지자체에서 자체적으로 보행안전법상 보행자길에 대한 전수조사를 자체적으로 실시할 수 있는지 여부에 대한 가능성을 살펴보았다. 이를 위해 실험 대상지 내 다양한 가로시설물 실측을 수행하여 드론촬영으로 획득된 포인트 클라우드 데이터를 기반으로 측정된 결과물의 정확도를 비교분석하였다. 분석결과 측정 오차범위가 공공측량 작업지침을 만족하는 것으로 나타났다. 고가의 장비나 소프트웨어를 제외하는 취지에서 무료오픈소스 프로그램으로 촬영결과를 분석하였으며, 실제 보도 관련 설계지침의 기준치들을 고려할 때 활용이 가능한 유의미한 결과를 도출하였다. 본 연구에서 제시한 방법론을 활용한다면, 향후 개별 지자체에서 보행환경개선을 위해 필요한 보행자길 전수조사를 용이하게 시행할 수 있을 것으로 보인다.

• Imaging Science in Dentistry
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• 제54권1호
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• pp.63-69
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• 2024

Purpose: The objective of this study was to determine the minimum number of teeth in the anterior dental arch that would yield accurate results for individual identification in forensic contexts. Materials and Methods: The study involved the analysis of 28 sets of 3-dimensional (3D) point cloud data, focused on the labial surface of the anterior teeth. These datasets were superimposed within each group in both genuine and imposter pairs. Group A incorporated data from the right to the left central incisor, group B from the right to the left lateral incisor, and group C from the right to the left canine. A comprehensive analysis was conducted, including the evaluation of root mean square error (RMSE) values and the distances resulting from the superimposition of dental arch segments. All analyses were conducted using CloudCompare version 2.12.4 (Telecom ParisTech and R&D, Kyiv, Ukraine). Results: The distances between genuine pairs in groups A, B, and C displayed an average range of 0.153 to 0.184mm. In contrast, distances for imposter pairs ranged from 0.338 to 0.522 mm. RMSE values for genuine pairs showed an average range of 0.166 to 0.177, whereas those for imposter pairs ranged from 0.424 to 0.638. A statistically significant difference was observed between the distances of genuine and imposter pairs(P<0.05). Conclusion: The exceptional performance observed for the labial surfaces of anterior teeth underscores their potential as a dependable criterion for accurate 3D dental identification. This was achieved by assessing a minimum of 4 teeth.

• 한국전자파학회논문지
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• 제29권3호
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• pp.233-240
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• 2018

레이다를 사용한 미사일 표적의 정확한 탐지 및 추적을 위해서는 채프 구름의 레이다 반사 단면적(Radar Cross Section: RCS)에 대한 분석이 반드시 필요하다. 따라서 본 논문에서는 다양한 환경에서 보다 효과적인 채프 구름의 RCS 분석을 위해 채프 구름 내 채프들을 개별적으로 계산하여 합하는 RCS 예측 방법과 공기역학 모델 기반의 확률밀도분포 모델을 사용한 RCS 예측 방법을 비교 및 분석하였다. 여기서, 상기 두 기법을 보다 더 정밀하게 비교 및 분석하기 위해 본 논문에서는 상용 전자기 수치해석 소프트웨어인 FEKO 7.0을 활용하여 반 파장 다이폴 형태의 단일 채프 CAD 모델의 RCS 값을 획득하여 채프 구름의 RCS를 모사하였다. 분석 결과, 확률 밀도 분포 모델을 사용한 경우 보다 효율적으로 체프 구름의 RCS 값을 예측할 수 있음을 확인하였다.