• 제목/요약/키워드: comparing region

검색결과 1,126건 처리시간 0.025초

칼라 영상에서의 중심 객체 추출에 관한 연구 (A Study on Extraction of Central Objects in Color Images)

  • 김성영;박창민;권규복;김민환
    • 한국멀티미디어학회논문지
    • /
    • 제5권6호
    • /
    • pp.616-624
    • /
    • 2002
  • 본 논문에서는 영상에 포함된 중심 객체를 추출하는 방법에 대해 제시한다. 중심 객체는 촬영의 중심이 되어 영상의 중앙 부분에 비교적 큰 면적을 차지하는 객체로 정의하는데 영상 내용에 대한 중요한 정보를 제공한다. 중심 객체 추출을 위해 우선 입력 영상에 대해 해상도를 줄여가며 영상 분할하고 분할된 결과에 대해 계층적 영역 병합을 수행함으로써 객체가 많은 수의 영역으로 세분화되어 영상 분할되는 것을 방지할 수 있도록 하였다. 분할된 각 영역은 영상의 경계와 접하는 경계 영역과 그 외의 비경계 영역으로 분류하였다. 비경계 영역은 중심 객체에 해당될 가능성이 있는 영역으로써, 이들 중에서 영상 중심 부근에서 가장 큰 크기를 차지하는 영역이 핵심객체영역으로 선택된다. 또한 경계 영역 중에서 영상의 네 모서리에 인접하는 영역은 핵심배경영역으로 선택되어 핵심객체영역과 함께 중심 객체 추출에 이용된다. 각 비경계 영역은 핵심 배경영역및 핵심객체영역과 칼라 분포 유사도출 비교하여 배경영역과 전경영역으로 분류된다. 핵심객체영역 및 핵심객체영역과 연결성을 가지는 전경영역이 최종 중심 객체로 선택된다. 본 논문에서 제안된 방법은 비교적 복잡한 배경을 갖는 영상에 대해서도 어느 정도 만족할 만한 결과를 얻을 수 있었다.

  • PDF

인공신경망을 이용한 공대지 유도폭탄의 투하가능영역 산출 (Computation for Launch Acceptability Region of Air-to-Surface Guided Bomb Using Artificial Neural Network)

  • 김성균;박정호;박상혁;이승필;김길훈
    • 한국항공우주학회지
    • /
    • 제46권4호
    • /
    • pp.283-289
    • /
    • 2018
  • 투하 가능 영역(LAR)은 표적에 성공적으로 명중하기 위한 영역을 의미하여, 항공기에서 실시간으로 계산되어 조종사가 인지할 수 있도록 시현해 주어야한다. LAR는 폭탄의 투하 조건, 표적의 탄착조건, 비행 시의 대기조건에 따라 변경된다. 본 논문에서는 인공신경망을 이용한 LAR 모델의 계산방법을 제시하였다. 기존의 LAR 모델에서 각 조건들을 변화하여 학습데이터를 생성하였으며, 인공신경망 학습을 통해 LAR 모델을 도출하였다. 기존 LAR 모델의 결과 데이터와 새로운 LAR 모델의 결과 데이터의 차이를 비교하여 모델의 정확도를 확인하였고, 계산시간을 비교하여 새로운 LAR 모델의 항공기에서 실시간 계산 가능성을 확인하였다.

Infectious bursal disease virus(국내분리주)의 variable VP2 gene의 분석 (Sequence analysis of the variable VP2 gene of infectious bursal disease viruses isolated in Korea)

  • 권혁무;김대규;성환우
    • 대한수의학회지
    • /
    • 제39권3호
    • /
    • pp.545-553
    • /
    • 1999
  • A 474-base pair segment covering the hypervariable region of VP2 gene from six Korean infectious bursal disease virus(K-IBDV) isolates(K1, K2, SH/92, 225, 269, 310) and one attenuated IBDV(DAE) were amplified using RT-PCR, sequenced, and compared with published sequences for IBDV. K-IBDV isolates(K1, K2, SH/92, 225, 269) and foreign very virulent(vv) IBDV strains had 94.93~100% amino acid sequence similarity. K-IBDV isolate 310 and other K-IBDV isolates had 84.31~86.07% amino acid sequence similarity. Attenuated strain(DAE), like other attenuated strain, has substitution at positions 279(D to N) and 284(A to T) as well as in the serine-rich heptapeptide region. Five K-IBDV isolates except 310 isolate share unique amino acid residues at positions 222(A), 256(I), 294(I) which are not present in other standard and attenuated strains. At the two hydrophilic region, K-IBDV isolates except 310 isolate had identical amino acids comparing with Belgium vv IBDV 894VB but had four amino acid substitutions comparing with Chinese vv IBDV F9502. The SWSASGS heptapeptide is conserved in all K-IBDV isolates. The sequence of K-IBDV isolate 310 was markedly different from other IBDV strains, evolving from a separate lineage than the others. By phylogenetic analysis, Five K-IBDV isolates except 310 isolate were categorized in one group with foreign vv IBDV isolates but K-IBDV isolate 310 was categorized in a separate group which was differentiated from other compared IBDV strains.

  • PDF

수도권 대학정원정책의 수동권 인구분산교과에 관한 연구 (University Enrollment Policy in the Capital Region and Its Impact on Population Dispersal)

  • 임창호;구자훈;안근원
    • 지역연구
    • /
    • 제9권1호
    • /
    • pp.45-63
    • /
    • 1993
  • University enrollment has long been regarded as one of the major factors inducing population concentration in Seoul and the Capital Region of Korea. Consequently, since early 1980's increases in enrollment and new establishments of extention universities beyond the boundary of Seoul, has been promoted, while university enrollment quota in Seoul has been strictly controlled. The degree of actual population dispersal, however, resulting from such a university enrollment policy has not been empirically tested. This paper aims at: First, identifying the trend of population growth and evolution process of the university enrollment policy in the Capital Region; Second, comparing the degree of influence of university enrollment on population concetration factors; Third, measuring actual effect of the enrollment control on population dispersal out of Seoul and the Capital Region. Major findings are as follows: First, only a week correlation between population and university enrollment growth trends was found; Second, the relative degree of influence on population concentration in the Capital Region, were order, in the order of magnitude, the physical amenity factor, the socio-cultural amenity factor, the employment climate factor and the educational factor. Third, and most improtant, based on the comparison of spatial distribution of graduated high schools and current residence of the selected university students, the gap between the two distributions was revealed and the inter-regional student population movement was estimated. The result shows that in Seoul's case about one-half of and in Kyunggi Province's case about one-fifth of university enrollment size, contributes to population concentration into Seoul. Fourth, as to the universities outside of the Capital Region, little effect in the case of universities located within the commuting distance, and a little effect on population dispersal in the case of universities located beyond commuting distance, were found. In sum, it seems clear that university enrollment policy in the Capital Region, especially in Inchon/Kyunggi Province has not been effective on student population dispersal out of Seoul and the Capital Region. Therefore, it is strongly recommended that university enrollment policy be throughly re-examined from its goal to the implementation means.

  • PDF

지역별 실업탈출확률 및 요인에 관한 연구 (Regional Analysis of Unemployment Hazard Rate and the Influencing Factors on It)

  • 정인수
    • 노동경제논집
    • /
    • 제26권1호
    • /
    • pp.111-151
    • /
    • 2003
  • 본 논문은 한국노동패널을 자료로, 위험도 모형 (hazard model)과 Cox 모형을 이용하여 실엽탈출확률 및 요인분석을 시도한 것이다. 실업탈출확률 분석의 결과, 수도권의 경우 실업률 수준 자체는 높지만 실업기간은 오히려 짧은 것으로 나타났다. 수도권과 비수도권 간의 분절성의 존재가 확인되었으며 경상도가 전라도 및 충청도에 비하여 실업탈출확률이 높게 나타나 경상도가 여타 지방과의 차이가 있다는 점도 확인되었다. 구체적으로는 수도권의 평균 실업기간이 9.29개월인 데 비하여 비수도권은 11.86개월로 수도권에서의 실업기간이 2.5개월(유의수준 0.001) 짧게 나타나 수도권에서의 실업탈출이 훨씬 수월함을 알 수 있었으며, 전라도 경상도 간의 차이를 보면, 평균 실업기간에서 전라도가 10.95개월 경상도가 6.96월로 4개월 정도로 전라도가 길게 유의하게 나타난다. 한편, 실업탈출에 영향을 주는 요인분석 결과를 보면, 대도시 이외의 지역, 비수도권 등 노동시장 취약지역에서는 여성일수록, 근속기간이 길수록, 임금근로자일수록, 제조업, 도소매업에 종사했던 근로자일수록 실업으로부터의 탈출확률이 낮아지고 있다. 위의 사실은 지역별 업종별 노동시장정책이 필요하며 특히 지역별 한계근로자에 대한 특성을 파악하여 새로운 직종이나 산업으로의 이동이 원활히 진행될 수 있도록 노동시장정책이 지역별로 보다 세밀히 수립 집행되어야 함을 시사한다.

  • PDF

이중 분무의 중첩 구조에 미치는 분무 노즐의 영향 (Effects of spray nozzles on the structure of twin spray)

  • 정종수;박찬범;임경수
    • 한국분무공학회지
    • /
    • 제1권3호
    • /
    • pp.51-59
    • /
    • 1996
  • An experiment was carried out on the structure of twin spray from pressurize-swirl nozzles, in order to investigate the effect of different size of spray nozzles on the characteristics of the overlap of two single sprays, for example, mean diameter, number density, and spatial distribution of flow rate. Using image processing method, the distributions of size and velocity of droplets of a single spray and twin spray were measured and compared to investigate the overlapping effect of two identical sprays. Comparing experimental results from a twin-spray with those from two-single sprays shows that the flow rate distribution of the twin-spray was concentrated around the midst of the overlapping region of two sprays. In this region, Sauter mean diameter (SMD) did not change much in the twin spray from 6032 nozzles, but it was smaller by 10 micrometers in the twin-spray than two-single sprays from 60063 nozzles. In spite of large difference in Weber numbers of the colliding sprays between the 60063 and 6032 nozzles, the phenomena did not have a big change in the overlapping region of twin spray. This shows that in the collision between droplets from two single spray in the overlapping region to cause the disruption of droplets, the size distribution of spray droplets was also important as well as Weber number.

  • PDF

딥 러닝 기반의 영상분할 알고리즘을 이용한 의료영상 3차원 시각화에 관한 연구 (Three-Dimensional Visualization of Medical Image using Image Segmentation Algorithm based on Deep Learning)

  • 임상헌;김영재;김광기
    • 한국멀티미디어학회논문지
    • /
    • 제23권3호
    • /
    • pp.468-475
    • /
    • 2020
  • In this paper, we proposed a three-dimensional visualization system for medical images in augmented reality based on deep learning. In the proposed system, the artificial neural network model performed fully automatic segmentation of the region of lung and pulmonary nodule from chest CT images. After applying the three-dimensional volume rendering method to the segmented images, it was visualized in augmented reality devices. As a result of the experiment, when nodules were present in the region of lung, it could be easily distinguished with the naked eye. Also, the location and shape of the lesions were intuitively confirmed. The evaluation was accomplished by comparing automated segmentation results of the test dataset to the manual segmented image. Through the evaluation of the segmentation model, we obtained the region of lung DSC (Dice Similarity Coefficient) of 98.77%, precision of 98.45%, recall of 99.10%. And the region of pulmonary nodule DSC of 91.88%, precision of 93.05%, recall of 90.94%. If this proposed system will be applied in medical fields such as medical practice and medical education, it is expected that it can contribute to custom organ modeling, lesion analysis, and surgical education and training of patients.

GALACTIC ANTICENTER CO SURVEY: I. L = $178^{\circ}$ TO $186^{\circ}$, B = $3^{\circ}.5$ TO $6^{\circ}.0$

  • LEE Y.;JUNG J. H.;CHUNG H. S.;PARK Y. S.;KIM H. R.;KIM H. G.;KIM B. G.;KIM J. S.;HAN S. T.
    • 천문학회지
    • /
    • 제29권spc1호
    • /
    • pp.173-174
    • /
    • 1996
  • We have mapped $17 deg^2$ region toward Galactic anticenter in $^{12}CO$ J = 1 - 0 using the 3 mm SIS receiver on the 14 m telescope at Taeduk Radio Astronomy Observatory (TRAO). The region mapped in this paper is the first target of the Galactic AntiCenter CO Survey Project (GACCOS) and was selected comparing with IRAS Sky Survey Atlas (ISSA) images at 100${\mu}m$. Molecular emission of the target area is found to be very extended and is well matching with the FIR emission boundary. There are several pieces of clouds, and as some of spectra show several peaks, there seem to be several clouds overlapped in some directions. The Velocity of Local Standard of Rest ($V_{LSR}$) of the CO emission of the mapped region ranges from -20 to +10 km/s. It is also found that the two cloudlets located around I = $180^{\circ}$ have $V_{LSR}$ = -20 km/s, which is very abnormal. The peak antenna temperature of 13 K arises near the H II Region S241.

  • PDF

FUV Observations of The Taurus-Auriga-Perseus complex

  • 임태호;민경욱;박재우;김일중;박성준;임여명;이대희;선광일
    • 천문학회보
    • /
    • 제35권1호
    • /
    • pp.71.1-71.1
    • /
    • 2010
  • We present the FUV continuum map of The Taurus-Auriga-Perseus complex, which is one of the largest local association of dark clouds. The map is well consistent with the dust extinction and the CO emission map of the T-P-A region. The region is divided into 3 sub-regions by diffuse FUV intensities and the spectra of each region imply that the radiation field due to the Per OB2-association can be a main source of the H2 fluorescent emission of the nearby cloud region. We used the PDR H2 model, named CLOUD, developed by van Dishoeck &Black for the sake of comparing our results to the H2 model.

  • PDF

Internal structure of a massive star-forming region G33.92+0.11 revealed by the high resolution ALMA observations

  • Minh, Young Chol;Liu, H.B.;Chen, H.R.
    • 천문학회보
    • /
    • 제43권1호
    • /
    • pp.44.2-44.2
    • /
    • 2018
  • G33.92+0.11, classified as a core-halo UC HII region at a distance of 7.1 kpc, contains several sub-clumps (~20-200 solar masses) as identified by dust continuum emission. This source shows very complicated features associated with vigorous massive star-forming activities with a nearly face-on projection. The ambient gas is still accreting to the massive molecular clumps dynamically, while the whole cloud is under disruption by newly formed stars. Using the recent high resolution (< 0.2") ALMA observations, we investigate the detailed structure associated with the star-forming activities by comparing different chemical tracers. The sub-clumps having extremely complex morphologies still preserve cold dense gas together with the turbulent and dense warm gas resulted by newly formed stars and interaction with accreting gas. The accretion of the ambient gas may have occurred episodically to this source. Most recent star formation, which probably the third generation of star formation in this region, is taking place in the northern part (A5 clump). The relatively small mass (~ 1/3 of A1 or A2) and the lack of turbulent gas of this star-forming core may suggest that this core was formed already during the overall collapse of the whole cloud for the first star formation. We think that gravitational collapse of these sub-clumps appears as sequential star formation of this region. The later interaction with accreting gas may have not been a direct cause of the star formation activities of this source.

  • PDF