• 한국환경과학회지
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• 제25권5호
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• pp.673-681
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• 2016

The adequacy of urban air quality monitoring networks in the largest metropolitan city, Seoul was evaluated using multivariate analysis for $SO_2$, $NO_2$, CO, PM10, and $O_3$. Through cluster analysis for 5 air pollutants concentrations, existing monitoring stations are seen to be clustered mostly by geographical locations of the eight zones in Seoul. And the stations included in the same cluster are redundantly monitoring air pollutants exhibiting similar atmospheric behavior, thus it can be seen that they are being operated inefficiently. Because monitoring stations groups representing redudancy were different depending on measurement items and several pollutants are being measured at the same time in each air monitoring station, it is seemed to be not easy to integrate or transmigrate stations. But it may be proposed as follows : the redundant stations can be integrated or transmigrated based on ozone of which measures are increasing in recent years and alternatively the remaining pollutants other than the pollutant exhibiting similar atmospheric behavior with nearby station's can be measured. So it is considered to be able to operate air quality monitoring networks effectively and economically in order to improve air quality.

• 지능정보연구
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• 제20권2호
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• pp.73-92
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• 2014

기존 협업 필터링 기법은 사용자들의 아이템에 대한 선호도를 기반으로 유사 아이템 집합 또는 유사 사용자 집합을 구성하고, 이를 이용해 예측된 사용자의 특정 아이템에 대한 선호도를 기반으로 추천을 수행한다. 이로 인해, 사용자 선호도 정보가 부족하게 되면, 유사 아이템 사용자 집합의 신뢰도가 낮아지고, 추천 서비스의 신뢰도 또한 따라서 낮아진다. 또한, 서비스의 규모가 커질수록, 유사 아이템, 사용자 집합의 생성에 걸리는 시간은 기하급수적으로 증가하고 추천서비스의 응답시간 또한 그에 따라 증가하게 된다. 위와 같은 문제점을 해결하기 위해 본 논문에서는 적응형 군집화 기법을 제안하고 이를 적용한 협업 필터링 기법을 제안하고 있다. 이 기법은 크게 네 가지 방법으로 이루어진다. 첫째, 사용자와 아이템의 특성 벡터를 기반으로 사용자와 아이템 각각을 군집화 하여, 기존 협업 필터링 기법에서 유사 아이템, 사용자 집합을 생성하는데 소요되는 시간을 절약하며, 사용자 선호도 정보만을 이용한 부분 집합 생성보다 추천의 신뢰도를 높이고, 초기 평가 문제와 초기 이용자 문제를 일부 해소한다. 둘째, 미리 구성된 사용자와 아이템의 군집을 기반으로 군집간의 선호도를 이용해 추천을 수행한다. 사용자가 속한 군집의 선호도가 높은 순서대로 아이템 군집을 조회하여 사용자에게 제공할 아이템 목록을 구성하여, 추천 시스템의 부하 대부분을 모델 생성 단계에서 부담하고 실제 수행 시 부하를 최소화한다. 셋째, 누락된 사용자 선호도 정보를 사용자와 아이템 군집을 이용하여 예측함으로써 협업 필터링 추천 기법의 사용자 선호도 정보 희박성으로 인한 문제를 해소한다. 넷째, 사용자와 아이템의 특성 벡터를 사용자의 피드백에 따라 학습시켜 아이템과 사용자의 정성적 특성 정량화의 어려움을 해결한다. 본 연구의 검증은 기존에 제안되었던 하이브리드 필터링 기법들과의 성능 비교를 통해 이루어졌으며, 평가 방법으로는 평균 절대 오차와 응답 시간을 이용하였다.

• 디지털산업정보학회논문지
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• 제6권4호
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• pp.11-20
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• 2010

Ontology is important role in semantic web to construct and query semantic data. Because of dynamic characteristic of ontology, P2P environment is considered for ontology processing in web environment. For efficient processing of ontology in P2P environment, clustering of peers should be considered. When new peer is added to the network, cluster allocation problem of the new peer is important for system efficiency. For clustering of peers with similar chateristics, similarlity measure method of ontology in added peer with ontologies in other clusters is needed. In this paper, we propose similarity measure techniques of ontologies for clustering of peers. Similarity measure method in this paper considered ontology's strucural characteristics like schema, class, property. Results of experiments show that ontologies of similar topics, class, property can be allocated to the same cluster.

• Industrial Engineering and Management Systems
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• 제8권2호
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• pp.101-108
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• 2009

Biclustering is a method to extract subsets of objects and features from a dataset which are characterized in some way. In contrast to traditional clustering algorithms which group objects similar in a whole feature set, biclustering methods find groups of objects which have similar values or patterns in some features. Both in clustering and biclustering, validating how much the result is informative or reliable is a very important task. Whereas validation methods of cluster solutions have been studied actively, there are only few measures to validate bicluster solutions. Furthermore, the existing validation methods of bicluster solutions have some critical problems to be used in general cases. In this paper, we review several well-known validation measures for cluster and bicluster solutions and discuss their limitations. Then, we propose several improved validation indices as modified versions of existing ones.

• 기술혁신연구
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• 제13권3호
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• pp.225-255
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• 2005

The similar point of the 19 regional industrial clusters of Japan is that all of the clusters are not limited to an administrational district but rather covers a larger area. When a cluster covers a larger area, there is problem of acquiring responsible businesses and interactive planing. In order to overcome such a problem, private coordinating organizations have been installed and operated to connect and manage inter-activities of industries, universities, and research institutes. TAMA, a private coordinating organization, differs from other associations in a way that it does not deal with one specific field or business. TAMA rather dealswith various product-developing small to middle size companies by offering strategic support for the development of new technologies and expansion of new businesses. Product-developing small to middle size companies comparatively have their own abilities for technological development and marketing which is quite different from other subcontract companies and their relations to large corporations. In such aspect, product-developing companies are actually similar to large corporations with competitiveness in the world market.

• 한국환경과학회지
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• 제17권5호
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• pp.517-524
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• 2008

The purpose of this study was to investigate the characteristics of air quality using data from which obtain local air quality monitoring system for cohort study in Chungju, Korea. We analyzed the concentration data of $NO_2,\;SO_2$, and $PM_{10}$ in Chungju and industrial cities in 2006. We compared a industrial area with a cohort study area using by bicluster algorithm. In the case of $SO_2$, the rate of the cluster time was $10{\sim}60%$ and the cluster time number of two areas was similar. In the case of $NO_2$ and $PM_{10}$, the number of cluster time between a industrial area and cohort study area was clearly different.

• 지식경영연구
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• 제15권4호
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• pp.147-170
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• 2014

This study investigates the main characteristics of Chinese automobile industry based on the technology learning, architecture theory and cluster. As a case study sample, we chose three most representative automobile firms from three main cities in China, FAW from northern part of China, SAIC from middle part of China, and BYD from southern part of China. According to the research findings, FAW has equipped self-production ability in virtue of political support but felled behind in future transportation due to lack of convergence with local cluster. In case of SAIS, similar phenomenon happened in spite of highest purchasing power of shanghai. BYD has achieved great quantum jump through the aggressive investment strategy in electric vehicle even though there are still many technological learning and experience to be cumulated. Overall, this research extends the current literature on key roles (technological learning, architecture, and cluster features) in the automobile industry growth by suggesting their crucial aspects in knowledge management and strategic planning to a newly emerging market, China, and sheds light on the relationship between regional characteristics and automobile growth.

• 한국인터넷방송통신학회논문지
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• 제10권2호
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• pp.25-30
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• 2010

무선 센서 네트워크는 제한된 자원을 가지고 특정한 지역에 임의로 뿌려진 센서 노드가 자가 구성적으로 형성하는 네트워크를 말한다. 센서 네트워크의 확장성(scalability), 로드 밸런싱(load balancing) 그리고 네트워크 라이프타임(network lifetime)을 보장하기 위해서 네트워크를 지역적으로 관리하는 클러스터링 알고리즘이 필요하다. 이전의 클러스터링 알고리즘에서 클러스터 헤드를 선정할 때 노드의 위치 및 에너지를 알아내기 위해 추가적인 통신비용이 발생하고, 클러스터 간 불균형이 클러스터 헤드에게 과부하를 유발한다. 따라서 본 논문은 이러한 문제점들을 해결하기 위해 추가적인 통신비용과 클러스터 불균형을 고려하는 새로운 클러스터 헤드 선정 알고리즘을 제안한다. 제안된 알고리즘은 실험결과를 통해 기존의 방법보다 에너지 측면에서 효율적임을 보여준다.

• 천문학회지
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• 제40권4호
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• pp.157-160
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• 2007

I present a model to explain the mass segregation and shallow mass functions observed in the central parts of starburst stellar clusters. The model assumes that the initial pre-stellar cores mass function resulting from the turbulent fragmentation of the proto-cluster cloud is significantly altered by the cores coalescence before they collapse to form stars. With appropriate, yet realistic parameters, this model based on the competition between cores coalescence and collapse reproduces the mass spectra of the well studied Arches cluster. Namely, the slopes at the intermediate and high mass ends, as well as the peculiar bump observed at $6M_{\bigodot}$. This coalescence-collapse process occurs on a short timescale of the order of the free fall time of the proto-cluster cloud (i.e., a few $10^4$ years), suggesting that mass segregation in Arches and similar clusters is primordial. The best fitting model implies the total mass of the Arches cluster is $1.45{\times}10^5M_{\bigodot}$, which is slightly higher than the often quoted, but completeness affected, observational value of a few $10^4M_{\bigodot}$. The model implies a star formation efficiency of ${\sim}30$ percent which implies that the Arches cluster is likely to a gravitationally bound system.

• 천문학회보
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• 제36권2호
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• pp.117.2-117.2
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• 2011

We probe 12CO J=2-1 and 13CO J=1-0 properties of a Virgo disk galaxy, NGC 4402 which is located near the cluster center. Our goal is to study the impact of intra cluster medium (ICM) on the molecular gas of a galaxy in the cluster environment. It has been believed that cluster galaxies are deficient in atomic hydrogen gas (HI gas) compared to their field counterparts and now there is much evidence that low density ISM can be easily removed by ram pressure caused by ICM wind. Meanwhile, no significant molecular gas deficiency of the cluster galaxy population has been found yet they show overall lower star formation rate than galaxies in the field, and it is still controversy whether dense ISM can be also stripped by the ICM wind or not. NGC 4402 with truncated HI disk($D_{HI}/D_{opt}$ ~ 0.75 and only 36%of HI gas compare to field galaxies of a similar size) and a disturbed gas morphology, appears to have strong ongoing ram pressure. Using high resolution 12 and 13CO data of NGC 4402 from a Sub Millimeter Array (SMA), we probe the molecular gas properties under strong ICM pressure. We discuss how its star formation activity and hence the global color of NGC4402 would be changed in the future.