PURPOSES : Traffic situation of Seoul City is different each administrative district. because each administrative district population, average travel speed, etc are different. thus, regionally differentiated policy is necessary. METHODS : In this study, first, it is to implement the cluster analysis using the traffic factor of twenty-five administrative districts in Seoul, categorize it into the cluster and understand the properties. second, related factors of speed were derived. and method to increase the speed was investigated. we choose the eleven traffic factors such as the number of traffic accident cases, total length, speed, the number of cross section, the number of cross section per km, the rate of roads, registered cars, population attending office and school, population density, area. RESULTS : In the results, first, we could categorize the Seoul-City administrative district into three clusters. in order to find Factors associated with speed a simple regression analysis was performed. and the number of intersections per km is closely related to the speed. CONCLUSIONS : Through this study, transportation policies reflecting local traffic-related characteristics are required.

본 연구는 딸기 ‘설향’ 품종의 화방별 착과순서에 따른 과중 및 당도의 변화를 조사하여 각 화방별로 착과량 조절 기준의 타당성을 검정하고자 하였다. 1화방은 2, 3화방에 비하여 착과수, 과중, 당도, 대과성 과실의 비율이 높았다. 동일 화방 내에서도 상위 과실은 하위에 착과된 과실보다 과중이 증가하였고 당도도 높았다. 과실의 과중이 증가할수록 당도가 증가하여 과중과 당도는 높은 정의 상관관계를 보였다. 설향 품종의 각 화방별 적정 착과수는 1화방 9∼10개, 2화방 6개, 3화방 4개, 4화방 3개 정도 착과시키는 것이 상품 수량을 증가시킬 수 있을 것으로 생각된다.

In the region of the open cluster M48 (NGC 2548), time-series BV CCD images were taken for 22 nights from February 28 in 2008 to March 17 in 2011. From this observation, we found 10 new variable stars. They include five eclipsing binaries, an RR Lyrae, two δ Scuti, and two semi-periodic and/or slow irregular type variable stars. We fail to find the member stars of the open cluster among the 10 variable stars.

We examine the dependence of the morphology of spiral galaxies on the environment using the KIAS Value Added Galaxy Catalog (VAGC) which is derived from the Sloan Digital Sky Survey (SDSS) DR7. Our goal is to understand whether the local environment or global conditions dominate in determining the morphology of spiral galaxies. For the analysis, we conduct a morphological classification of galaxies in 20 X-ray selected Abell clusters up to z~0.06, using SDSS color images and the X-ray data from the Northern ROSAT All-Sky (NORAS) catalog. We analyze the distribution of arm classes along the clustercentric radius as well as that of Hubble types. To segregate the effect of local environment from the global environment, we compare the morphological distribution of galaxies in two X-lay luminosity groups, the low-Lx clusters (Lx < 0.15 X 1044erg/s) and high-Lx clusters (Lx > 1.8 X 1044erg/s). We find that the morphology-clustercentric relation prevails in the cluster environment although there is a brake near the cluster virial radius. The grand design arms comprise about 40% of the cluster spiral galaxies with a weak morphology-clustercentric radius relation for the arm classes, in the sense that flocculent galaxies tend to increase outward, regardless of the X-ray luminosity. From the cumulative radial distribution of cluster galaxies, we found that the low-Lx clusters are fully virialized while the high-Lx clusters are not.

여름에 바다로부터 불어오는 해풍은 해안 도시지역에서의 열섬현상을 감소하기 위한 방법 중 하나로 제시되었다. 특히 바람을 이용한 열섬 효과 저감은 해풍의 특성 -연직 풍속 및 온도 분포- 에 많이 영향을 받는다. 따라서, 열섬 효과 저감을 위한 도시 개발단계에서 해풍을 이용하기 위해서는 해풍의 특성을 충분히 이해해야만 한다. 본 연구에서는 대기 기상 모델링을 이용하여 동경 지역을 수치 해석을 하였다. 수치 해석 결과를 클러스터 분석을 통하여 8개의 대표적인 해풍의 연직 패턴을 분류하였으며, 각 분류된 패턴간의 관계 및 발생 빈도를 비교 및 검토하였다.

UBV I CCD photometry of NGC 2353 is performed as a part of the "Sejong Open cluster Survey" (SOS). Using photometric membership criteria we select probable members of the cluster. We derive the reddening and distance to the cluster, i.e., E(B - V ) = 0.10 ± 0.02 mag and 1.17 ± 0.04 kpc, respectively. We find that the projected distribution of the probable members on the sky is elliptical in shape rather than circular. The age of the cluster is estimated to be log(age)=8.1 ± 0.1 in years, older than what was found in previous studies. The minimum value of binary fraction is estimated to be about 48 ± 5 percent from a Gaussian function fit to the distribution of the distance moduli of the photometric members. Finally, we also obtain the luminosity function and the initial mass function (IMF) of the probable cluster members. The slope of the IMF is Γ = -1.3 ± 0.2.

We study near-infrared properties of the old open cluster King 11, based on the 2MASS photometric data. We determine the location of the red giant clump(RGC) in the (K, J - K) colo-magnitude diagram and derive the distance modulus of King 11 to be (m-M)0 = $12.50 ± 0.10 using the mean K magnitude of RGC. From the red giant branch slope - [Fe/H] relation we obtain the metallicity of this cluster, [Fe/H]=-0.17±0.07. The age and interstellar reddening of this cluster are estimated to be log t = 9.48±0.05, E(B-V)=0.90±0.03, by applying Padova isochrone fits to the data.