• 한국컴퓨터그래픽스학회논문지
• /
• 제29권4호
• /
• pp.17-24
• /
• 2023

컴퓨터 그래픽스 및 컴퓨터 비전 분야의 발전에 따라 삼차원 물체를 다양한 표현 방식으로 나타내고 있다. 이에 따라 여러 표현 방식을 사용하는 캐릭터의 애니메이션 제작에 대한 수요 또한 증가하고 있다. 캐릭터 애니메이션 제작에 주로 사용되는 스켈레탈 애니메이션의 경우 캐릭터 표면이 어느 관절로부터 영향을 받는지를 정하는 스키닝 웨이트 페인팅 작업이 필요하다. 본 논문은 삼각형 메시를 비롯한 여러 표현방식으로 나타난 캐릭터에 대한 스키닝 웨이트 페인팅 과정을 자동화하는 방법을 제안한다. 우선 다양한 표현 방식을 사용한 삼차원 캐릭터에 대해 일반적으로 사용할 수 있도록 Signed Distance Field(SDF)를 이용한다. 이후 그래프 신경망과 다층 퍼셉트론 계층 구조를 활용하여 캐릭터 표면 상에 주어진 위치에서의 스키닝 웨이트를 예측할 수 있다.

• 한국가스학회지
• /
• 제2권3호
• /
• pp.12-17
• /
• 1998

공정의 위험성 평가를 위한 이상트리 작성은 많은 시간과 인력을 요하는 작업으로 대규모 화학공장에 적용하기가 매우 힘들다. 본 연구에서는 화학공정의 이상트리 합성을 위해서, 공정변수간의 인과관계를 나타내는 부호 유향그래프로 발생 가능한 모든 공정이상과 원인들을 표현하고, 부호 유향그래프상에 존재하는 경로특성에 따라 일반 조작자와 루프 조작자를 정의하여 이상사건의 원인을 탐색할 때 해당하는 경로의 특성에 맞는 조작자로 대치함으로써 이상트리를 자동합성하였다.

• 한국지능시스템학회:학술대회논문집
• /
• 한국퍼지및지능시스템학회 1997년도 추계학술대회 학술발표 논문집
• /
• pp.247-251
• /
• 1997

FCM(Fuzzy Cognitive Map) is a fuzzy signed directed graph for representing causal reasoning which has fuzziness between causal concepts. Authors have already proposed FCM-based fault diagnostic scheme and verified its usefulness. However, the previously proposed scheme has the problem of lower diagnostic resolution as in the case of other qualitative approaches. In order to improve the diagnostic resolution, a concept of fuzzy number is introduced into the basic FCM-based fault diagnostic algorithm. By incorporation the fuzzy number into fault FCM models, quantitative information such as the transfer gain between the state variables can be effectively utilized for better diagnostic resolution. Furthermore, an enhanced TAM(Temporal Associative Memory) recall procedure and modified and modified pattern matching scheme are also proposed.

• 한국안전학회지
• /
• 제11권3호
• /
• pp.104-111
• /
• 1996

A system was developed that could predict hazardous states for safe operation of chemical plants. This system aimed to prevent hazards of chemical processes from misoperation before real operation. In this study, a data base was organized which consisted of all hazards in the chemical processes. The structure of process was represented by signed direct graph(SDG) of NODEs and ARCs. Each NODE and ARC have property variables ; connected structure and state of processes etc. The hazards that could be occurred in processes were divided into two classes ; one is by operation of unit and the other is by hazardous materials. Using Hazardous States Transition Network, we could recognize transition progress of process states.

• 제어로봇시스템학회:학술대회논문집
• /
• 제어로봇시스템학회 1993년도 한국자동제어학술회의논문집(국내학술편); Seoul National University, Seoul; 20-22 Oct. 1993
• /
• pp.233-238
• /
• 1993

In this paper, two diagnosis algorithms using the simple fuzzy, cognitive map (FCM) that is an useful qualitative model are proposed. The first basic algorithm is considered as a simple transition of Shiozaki's signed directed graph approach to FCM framework. And the second one is an extended version of the basic algorithm. In the extension, three important concepts, modified temporal associative memory (TAM) recall, temporal pattern matching algorithm and hierarchical decomposition are adopted. As the resultant diagnosis scheme takes short computation time, it can be used for on-line fault diagnosis of large scale and complex processes that conventional diagnosis methods cannot be applied. The diagnosis system can be trained by the basic algorithm and generates FCM model for every experienced process fault. In on-line application, the self-generated fault model FCM generates predicted pattern sequences, which are compared with observed pattern sequences to declare the origin of fault. In practical case, observed pattern sequences depend on transport time. So if predicted pattern sequences are different from observed ones, the time weighted FCM with transport delay can be used to generate predicted ones. The fault diagnosis procedure can be completed during the actual propagation since pattern sequences of tvo different faults do not coincide in general.

• 한방재활의학과학회지
• /
• 제32권1호
• /
• pp.51-62
• /
• 2022

Objectives Objective of this study is to investigate the role of paraspinal muscles by examining the correlation between slip percentage (SP) of spondylolisthesis and fatty infiltration of lumbar paraspinal muscle. Methods Retrospective analysis was performed on 45 patients diagnosed with spondylolisthesis based on medical records. Using T2-weighted axial magnetic resonance imaging, cross-sectional areas (CSAs) of psoas major (PM), multifidus (MU) and erector spinae (ES) were calculated and divided by CSA of lower level vertebral body (VB). SP was measured using sagittal T2-weighted images. Correlation of SP with muscle relative cross-sectional area (RCSA) and muscle fatty infiltration by Goutallier classification was respectively analyzed using Spearman correlation. Statistic assessment conducted by Wilcoxon signed rank test and paired t-test using program GraphPad prism 5 (GraphPad Software, Inc., San Diego, CA, USA). Results Spondylolisthesis forward slip percentage by Taillard's method was negatively associated with both side MU RCSAs. No significant correlation was found between PM RCSA, ES RCSA and SP. Forward slippage was significantly correlated with fatty infiltration of lumbar paraspinal muscle measured by Goutallier classification. Conclusions This study is to understand the role of paraspinal muscle affecting spinal instability by investigating correlation between statistical deviation of lumbar muscle characters (RCSA, fatty infiltration of lumbar muscle) and SP. We found that spondylolisthesis SP is positively related to fatty infiltration of lumbar paraspinal muscle. and is negatively associated with both side MU RCSAs.

• 한방재활의학과학회지
• /
• 제32권3호
• /
• pp.119-129
• /
• 2022

Objectives This study aimed to evaluate the effects of Integrative treatment of traditional Korean medicine (TKM) on 7 hospitalized patients after hip fracture surgery, and to identify significant herbs and co-prescribed herbs by using network analysis and association rule mining. Methods A retrospective chart review of the 7 hospitalized patients treated for postoperative hip fractures between January and December 2021 was performed. All TKM treatments for the patients were identified and Wilcoxon signed-rank test was performed to compare hip pain and mobility on admission and discharge. We visualized the network of herbal medicines and complications. By using network analysis, we also identified the significant herbs (high centrality of degree, eigenvector, and sub-graph). Co-prescription patterns for the hip fracture patients were further analyzed by association rule mining. Results We found that TKM treatment significantly relieved hip pain and improved mobility. Accompanying symptoms reported by the patients were general weakness, anorexia, dizziness, delirium, edema, sputum, sore throat, cough, rhinorrhea, and chills. Herbs composed of Sagunja-tang and Samul-tang showed high centralities and high associations with other herbs. In addition, Gupan, Nokyong, Yukjongyong, Useul, and Hyunhosaek were identified as important herbs for postoperative hip fracture patients. Conclusions This study provides evidence for clinical TKM use as an effective postoperative treatment for pain relief and improvement of mobility in patients with hip fractures. In addition, herbs that can be considered in the treatment of patients after hip fracture surgery were identified through network analysis and association rule mining.

• 핵의학기술
• /
• 제14권2호
• /
• pp.26-32
• /
• 2010

핵의학 체내검사 업무 단계 별 작업종사자의 피폭선량을 측정 및 분석하여 환자 검사 및 업무효율 저하를 발생시키지 않는 범위 내에서 종사자의 피폭선량을 최소로 감소할 수 있는 방법을 알아보고자 하였다. 방사성동위원소를 이용한 핵의학 체내검사 업무는 방사성 동위원소 분배, 방사성동위원소 주사($^{99m}Tc$, $^{18}F$-FDG), 환자 안내 및 검사로 이루어진다. RadEye-G10 측정기기(Thermo SCIENTIFIC)를 이용하여 각 업무 단계 별 피폭선량을 측정 및 분석 하였다. 방사성동위원소를 환자에게 주사하는 과정에서 많은 피폭이 발생하므로 작업종사자의 피폭선량을 최소로 줄일 수 있도록 외부피폭 방어에 대한 교육과 방사성동위원소 주사 시 보호구를 착용하도록 하였으며 주사 전 검사에 대한 설명 및 주의사항을 교육하여 주사 후 환자와의 대면시간을 단축하여 피폭선량을 줄이도록 하였다. 방사성동위원소 주사 시 보호구 착용 유무에 따른 피폭선량과 주사 전 검사에 대한 설명 및 주의사항 교육 유무에 따른 피폭선량을 측정하였다. 총 피폭선량은 icrosoft office Excel 2007을 이용하여 그래프로 나타내었으며 피폭선량의 차이는 SPSS program 12.0을 이용하여 wilcoxon signed ranks test로 분석 하였다. 이 때 p값이 0.01 이하인 경우 통계적으로 유의 하다고 판단하였다. $^{99m}Tc$-DPD 20 mCi를 보호구를 착용하고 주사 시 피폭되는 선량은 보호구를 착용하지 않고 주사 시 피폭되는 선량보다 88% 감소하였으며 통계적으로 유의한 차이가 있었다 (p<0.01). $^{18}F$-FDG 10 mCi를 보호구를 착용하고 주사 시 피폭되는 선량은 보호구를 착용하지 않고 주사 시 피폭되는 선량보다 26% 감소하였으나 통계적으로 유의한 차이는 없었다(p>0.01). $^{99m}Tc$-DPD 20 mCi를 주사 전 검사에 대한 설명 및 주의사항 교육 시 피폭되는 선량은 주사 후 검사에 대한 설명 및 주의사항 교육 시 피폭되는 선량보다 63% 감소하였으며 통계적으로 유의한 차이가 있었다(p<0.01). $^{18}F$-FDG 10 mCi를 주사 전 검사에 대한 설명 및 주의사항 교육 시 피폭 되는 선량은 주사 후 검사에 대한 설명 및 주의사항 교육 시 피폭되는 선량보다 52% 감소하였으며 통계적으로 유의한 차이가 있었다(p<0.01). 방사성동위원소 $^{99m}Tc$을 이용하는 검사에서는 보호구 착용이 피폭선량을 줄이는데 더 효과적이고 $^{18}F$-FDG를 이용하는 검사에서는 주사 후 환자와의 대면시간을 단축하는 것이 피폭선량을 줄이는데 더 효과적이다. 그러므로 이러한 방사성동위원소의 특성에 따라 차폐 방안을 모색한다면 더욱 더 효과적이고 적극적인 방사선 차폐가 될 것으로 사료된다.

• 천문학회지
• /
• 제29권spc1호
• /
• pp.63-64
• /
• 1996

The nature of distant faint blue field galaxies remains a mystery, despite the fact that much attention has been devoted to this subject in the last decade. Galaxy counts, particularly those in the optical and near ultraviolet bandpasses, have been demonstrated to be well in excess of those expected in the 'no-evolution' scenario. This has usually been taken to imply that galaxies were brighter in the past, presumably due to a higher rate of star formation. More recently, redshift surveys of galaxies as faint as B$\~$24 have shown that the mean redshift of faint blue galaxies is lower than that predicted by standard evolutionary models (de-signed to fit the galaxy counts). The galaxy number count data and redshift data suggest that evolutionary effects are most prominent at the faint end of the galaxy luminosity function. While these data constrain the form of evolution of the overall luminosity function, they do not constrain evolution in individual galaxies. We are carrying out a series of observations as part of a long-term program aimed at a better understanding of the nature and amount of luminosity evolution in individual galaxies. Our study uses the luminosity-linewidth relation (Tully-Fisher relation) for disk galaxies as a tool to study luminosity evolution. Several studies of a related nature are being carried out by other groups. A specific experiment to test a 'no-evolution' hypothesis is presented here. We have used the AUTOFIB multifibre spectro-graph on the 4-metre Anglo-Australian Telescope (AAT) and the Rutgers Fabry-Perot imager on the Cerro Tolalo lnteramerican Observatory (CTIO) 4-metre tele-scope to measure the internal kinematics of a representative sample of faint blue field galaxies in the red-shift range z = 0.15-0.4. The emission line profiles of [OII] and [OIII] in a typical sample galaxy are significantly broader than the instrumental resolution (100-120 km $s^{-l}$), and it is possible to make a reliable de-termination of the linewidth. Detailed and realistic simulations based on the properties of nearby, low-luminosity spirals are used to convert the measured linewidth into an estimate of the characteristic rotation speed, making statistical corrections for the effects of inclination, non-uniform distribution of ionized gas, rotation curve shape, finite fibre aperture, etc.. The (corrected) mean characteristic rotation speed for our distant galaxy sample is compared to the mean rotation speed of local galaxies of comparable blue luminosity and colour. The typical galaxy in our distant sample has a B-band luminosity of about 0.25 L$\ast$ and a colour that corresponds to the Sb-Sd/Im range of Hub-ble types. Details of the AUTOFIB fibre spectroscopic study are described by Rix et al. (1996). Follow-up deep near infrared imaging with the 10-metre Keck tele-scope+ NIRC combination and high angular resolution imaging with the Hubble Space Telescope's WFPC2 are being used to determine the structural and orientation parameters of galaxies on an individual basis. This information is being combined with the spatially resolved CTIO Fabry-Perot data to study the internal kinematics of distant galaxies (Ing et al. 1996). The two main questions addressed by these (preliminary studies) are: 1. Do galaxies of a given luminosity and colour have the same characteristic rotation speed in the distant and local Universe? The distant galaxies in our AUTOFIB sample have a mean characteristic rotation speed of $\~$70 km $s^{-l}$ after correction for measurement bias (Fig. 1); this is inconsistent with the characteristic rotation speed of local galaxies of comparable photometric proper-ties (105 km $s^{-l}$) at the > $99\%$ significance level (Fig. 2). A straightforward explanation for this discrepancy is that faint blue galaxies were about 1-1.5 mag brighter (in the B band) at z $\~$ 0.25 than their present-day counterparts. 2. What is the nature of the internal kinematics of faint field galaxies? The linewidths of these faint galaxies appear to be dominated by the global disk rotation. The larger galaxies in our sample are about 2"-.5" in diameter so one can get direct insight into the nature of their internal velocity field from the $\~$ I" seeing CTIO Fabry-Perot data. A montage of Fabry-Perot data is shown in Fig. 3. The linewidths are too large (by. $5\sigma$) to be caused by turbulence in giant HII regions.