• 대한안전경영과학회지
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• 제6권3호
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• pp.77-86
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• 2004

Observational methods to evaluate postural load have an intrinsic week point that is the problem of reliability in observing postures subjectively, although they have been widely used in assessing risk factors of work-related musculoskeletal disorders in the industry. In this study, observational reliability was discussed based on reviewing several previous studies. Practical guidelines was presented to reduce the observational errors when using video recording for the assessment of risk factors. In addition, previous studies on observational reliability were summarized and analyzed according to body parts to be observed, media for observation, objective measures, analysis, statistics, etc. It is expected that this basic study can be used to increase the applicability and accuracy of the observational methods.

• 수산해양기술연구
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• 제34권1호
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• pp.21-29
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• 1998

In order to investigate the fish behavior in the water tank, the three dimensional positioning system with two CCD cameras was designed. The positioning system was tested at the vertical circulation water channel with observational part of 1,500L$\times$1,500W$\times$500H mm and the circular water tank with 2,050ø sub(1)$\times$1,850ø sub(2)$\times$400H mm. The observational error of vertical direction was larger than that of horizontal direction, and the observational error became enlarged in all directions according to the increase of depth and distance from the visual axis. The maximum observational errors of horizontal and vertical directions at the circulation channel ranged from -1.7 cm to 1.8 cm (2.4%) and zero to 2.1 cm (4.2%), respectively. But the errors of horizontal and vertical directions at the circular tank ranged from -1.3 cm to 1.3 cm (1.3%) and zero to 1.3 cm (3.3%), respectively.

• Journal of Astronomy and Space Sciences
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• 제21권4호
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• pp.361-370
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• 2004

본 연구에서는 행성간 탐사선의 정밀궤도결정에 필수적인 심우주 추적망(Deep Space Network, DSN) 관측모델을 개발하였다. DSN 관측모델은 DSN 관측시 발생하는 오차를 모델링하여 실제 DSN 관측값과 동일한 관측값을 생성하는 역할을 수행한다. 본 연구의 목적은 행성간 탐사선 정밀궤도결정 과정의 일환인 DSN 관측모델을 개발하는 것이다. DSN 관측모델에는 대류층, 이온층과 안테나 옵셋 오차 모델을 포함시켰으며 임무에 따라 변하는 파라미터 값도 적용하였다. 또한 DSN 관측모델을 3개의 DSN 지상국에서 방위각-고도 마운트를 사용하는 모든 안테나에 대해 구현하였다. 고려한 오차모델의 결과값과 JPL 결과값을 비교해 본 결과, 모든 오차모델 값이 JPL에서 제시한 허용오차 범위인 $10\%$ 내에 있음을 확인하였다. 오차모델과 파라미터를 고려하여 실제 관측과 동일한 DSN 관측값을 생성하였으며, 이를 통해 본 연구에서 개발된 관측모델이 향후 우리 나라 행성간 탐사 임무시 정밀궤도 결정을 위한 관측모델로 활용 가능함을 확인하였다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.38.2-38.2
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• 2008

In Korean historical documents, there are a great number of the records for various astronomical events. In particular, historical documents of the Joseon dynasty also have the records containing observational data by an astronomical instrument. However, a quantitative analysis for the accuracy of observational values have never been studied, although there are some studies on the truth of the records themselves. Hence, we investigated observation errors during the period of the Joseon dynasty from the records of Joseon-Wang-Jo-Sil-Lok (the Annals of the Joseon Dynasty) and Seung-Jeong-Won-Il-Gi (Daily Records of the Royal Secretariat). We used the records of the Mars, supernova 1604, and Halley's Comet, and found that observational values before the Hideyoshi invasions in 1592 are relatively more accurate than those after then. However, because the number of cases used in this study is small, we think that more studies are needed to confirm our results. Nonetheless, we reckon our work will be of service to understand astronomical records of the Joseon dynasty.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2002년도 Proceedings of International Symposium on Remote Sensing
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• pp.407-407
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• 2002

The most widespread techniques for DEM generation are stereoscopy for optical sensor images and interfereometry for SAR images. These techniques suffer from certain sensor and processing limitations, which can be overcome by the synergetic use of both sensors and DEMs respectively. In this paper, different strategies for fusing SAR and optical data are combined to derive high quality DEM products. The filtering techniques, which take advantage of the complementary properties of SAR and stereo optical DEMs, will be applied for the fusion process. By taking advantage of the fact that errors of the DEMs are of different nature using the filtering technique, affected part are filtered and replaced by those of the counterpart and is tested with two sets of SPOT and ERS DEM, resulting in a remarkable improvement in DEM. for the analysis of results, the reference DEM is generated from digital base map(1:5000).

• 한국지반공학회지:지반
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• 제14권2호
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• pp.41-54
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• 1998

지반의 불균질성, 토질상수의 측정에 연관된 오차. 압밀이론의 단점 등으로 예측된 압밀침하량 및 시간은 항상 실측치와 잘 일치하지 않게 된다. 압축성 지반 위에 성토가 이루어질 때, 최종 침하량과 압밀시간을 예측하기 위한 예측기법은 실무에서 유용한 수단이다. 그러나, 기존의 예측기법들에 의한 침하곡선에서 직선을 찾기가 어렵거나, 개인오차를 피할 수 없는 등의 단점을 내포하고 있다. 본 논문에서는 새로운 예측기법($\sqrt{s}$법)으로 현장에서 압밀해석을 수행하기 위하여 제안되었다. 두 현장에 대하여 $\sqrt{s}$-법과 함께 다른 기존의 방법들을 적용한 결과, $\sqrt{s}$법과 Asaoka법에 의해 예측된 최종침하량은 실측치와 좋은 일치를 보여주었으나, 쌍곡선법(Tan, 1991)에서는 항상 과대평가된 결과를 또한 Hoshino 법에서는 많은 경우에 예측이 불가한 결과를 보여주었다.$\sqrt{s}$- 법에 의한 침하곡 선상에서 평균압밀도가 60%와 90% 사이에서 직선을 나타내고 있어서 개인오차를 유발할 가능성이 희박하였다. $\sqrt{s}$- 법에 의하여 예측된 최종압밀시간은 실측치와 잘 일치하고 있는 반면에 Asaoka 와 Tan(1996) 방법에 의한 결과는 아주 과소평가되거나 과대평가되었다. 이러한 이유는 후자의 두 방법에서 단계성토의 영향이 고려되지 못했기 때문인 것으로 사료된다.

• ETRI Journal
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• 제11권4호
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• pp.22-36
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• 1989

In this paper, a design and implementation of an efficient protocol verification system named LOVE has been described. The LOVE has been developed specifically for LOTOS. It performs not only protocol syntax validation (PSV) but also protocol functional verification(PFV). The PSV is a test to check if a protocol is free from protocol syntax errors such as deadlocks and livelocks. The PFV confirms whether or not a protocol achieves its functional objectives. For the PSV, the reachability analysis is employed, and the observational equivalence test is used for the PFV. For protocol verification using the LOVE, a schematic protocol verification methodology has been outlined.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1993년도 한국우주과학회보 제2권2호
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• pp.19-19
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• 1993

We have developed a new method to simulate the observed color magnitudediagrams for Galactic globular clusters. The model calculations include all evolutionary phases- from zero age main sequence to asymptotic giant branch. Using these models, we can simulate directly the observational errors and sampling effect and also can examine the stellar evolution theory in more$.$ realistic way. Implications of these model calculations on the recent space observations of globular clusters and other systems will be discussed.

• 대기
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• 제33권1호
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• pp.33-47
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• 2023

In this study, for the application of observation errors to the Korean Integrated Model (KIM) to utilize the Constellation Observing System for Meteorology, Ionosphere & Climate-2 (COSMIC-2) new satellites, the observation errors were diagnosed based on the Desroziers method using the cost function in the process of variational data assimilation. We calculated observation errors for all observational species being utilized for KIM and compared with their relative values. The observation error of the calculated the Global Navigation Satellite System Radio Occultation (GNSS RO) was about six times smaller than that of other satellites. In order to balance with other satellites, we conducted two experiments in which the GNSS RO data expanded by about twice the observation error. The performance of the analysis field was significantly improved in the tropics, where the COSMIC-2 data are more available, and in the Southern Hemisphere, where the influence of GNSS RO data is significantly greater. In particular, the prediction performance of the Southern Hemisphere was improved by doubling the observation error in global region, rather than doubling the COSMIC-2 data only in areas with high density, which seems to have been balanced with other observations.

• Journal of Astronomy and Space Sciences
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• 제31권2호
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• pp.121-130
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• 2014

Essential ideas, successes, and difficulties of Areal Density Analysis (ADA) for color-magnitude diagrams (CMD's) of resolved stellar populations are examined, with explanation of various algorithms and strategies for optimal performance. A CMD-generation program computes theoretical datasets with simulated observational error and a solution program inverts the problem by the method of Differential Corrections (DC) so as to compute parameter values from observed magnitudes and colors, with standard error estimates and correlation coefficients. ADA promises not only impersonal results, but also significant saving of labor, especially where a given dataset is analyzed with several evolution models. Observational errors and multiple star systems, along with various single star characteristics and phenomena, are modeled directly via the Functional Statistics Algorithm (FSA). Unlike Monte Carlo, FSA is not dependent on a random number generator. Discussions include difficulties and overall requirements, such as need for fast evolutionary computation and realization of goals within machine memory limits. Degradation of results due to influence of pixelization on derivatives, Initial Mass Function (IMF) quantization, IMF steepness, low Areal Densities ($\mathcal{A}$), and large variation in $\mathcal{A}$ are reduced or eliminated through a variety of schemes that are explained sufficiently for general application. The Levenberg-Marquardt and MMS algorithms for improvement of solution convergence are contained within the DC program. An example of convergence, which typically is very good, is shown in tabular form. A number of theoretical and practical solution issues are discussed, as are prospects for further development.