• 제목/요약/키워드: space morphology

검색결과 296건 처리시간 0.024초

SiO IN THE SGR B2 REGION

  • Minh, Y.C.
    • 천문학회지
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    • 제40권3호
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    • pp.61-65
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    • 2007
  • The 2-1 and 5-4 transitions of SiO have been observed toward the Sgr B2 region, including the Principal Cloud(the GMC containing Sgr B2(M)) and its surroundings. The morphology and velocity structure of the SiO emission show a close resemblance with the HNCO Ring feature, identified by Minh & Irvine(2006), of about 10 pc in diameter, which may be expanding and colliding with the Principal Cloud. Three SiO clumps have been found around the Ring, with total column densities $N_{SiO}{\sim}1{\times}10^{14}cm^{-2}$ at the peak positions of these clumps. The fractional SiO abundance relative to $H_2$ has been estimated to be ${\sim}(0.5-1){\times}10^{-9}$, which is about two orders of magnitude larger than the quiet dense cloud values. Our SiO observational result supports the existence of an expanding ring, which may be triggering active star formations in the Principal Cloud.

알루미늄 합금의 랜덤하중 하에서 발생한 피로파면 해석 방법 (Fractographic Analysis Method of Fatigue Fracture Surface under Program and Random Loading for Aluminum Alloy)

  • 김상태;최성종;양현태;이희원
    • 대한기계학회논문집A
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    • 제27권12호
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    • pp.2055-2060
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    • 2003
  • Striation is a typical pattern observed on the fatigue fracture surface and the spacing is known to correspond to a macroscopic fatigue crack growth rate, and many models for the predict in the formation of such striation have been proposed. However, these theories and methods can't be applied under random loading spectrum. In this study, the fatigue tests were carried out on aluminum alloy under random loading spectrum. The fatigue fracture surfaces were observed in the scanning electron microscope (SEM) and great quantities of SEM micrographs were synthesized and saved in computer system. The space and morphology of several large-scale striations, which are expected to from at the relatively greater load range in loading block, were observed. The crack length for each loading blocks was decided in consideration of regularity and repetition of those striations. It is shown that the applicability of fractographic methods on the fatigue fracture surface under random loading spectrum.

Note on the Species of Ceramium (Ceramiace Rhodophyta) from Ullungdo Island, Korea

  • In Kyu Lee
    • Journal of Plant Biology
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    • 제38권2호
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    • pp.159-164
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    • 1995
  • The taxonomic note was given to the species of Ceramium from Ullungdo Island. Five species, Ceramium aduncum Nakamura, C. codii (Rhichards) G. Mazoyer, C. flaccidum (Harvey exK tzing) Ardissone, C. paniculatum Okamura, and C. tenerrimum (Martense) Okamura were collected during this study. C. aduncum was collected in the intertidal and upper subtidal zones from December to Feburary. They had a narrow internodal space showing 1/3-1/5 times as large as nodal band. C. codii had the spermatangial mother cells developed on abaxial cortical cells of cortical band C. paniculatum collected in summer and winter had a creeping thallus and alternative branching type in gross morphology. The axial cell of C. flaccidum showed 2.3-2.8 L/B ratio, smaller than those of plants from Chejudo Island.

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FUV Images and Physical Properties of the Orion-Eridanus Superbubble region

  • Ko, Young-Soo;Min, Kyoung-Wook;Seon, Kwang-Il
    • 천문학회보
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    • 제35권2호
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    • pp.71.1-71.1
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    • 2010
  • The far-ultraviolet (FUV) C IV and H2 emission spectra of Orion-Eridanus Superbubble (OES) is hereby presented. The OES seems to consist of multiple phase through the detection of highly-ionized gas and pervasive neutral hydrogen. The former is traced by hot gas while the latter is traced by cold medium. A spectral image made with H2 fluorescent emission shows that the spatial distribution of hydrogen molecule is well correlated with the dust map. The model spectra was taken from a photodissociation region (PDR) radiation code which finds a best suitable parameter such as hydrogen density and intensity of the radiation field. C IV emission is caused by intermediate temperature ISM about 10^5 K. Therefore we could get more clear evidence to reveal the morphology of OES. In this process, the hydrogen density and gas temperature were also estimated. The data were obtained with the Far-Ultraviolet Imaging Spectrograph (FIMS) and the whole data handling were followed by previous FIMS analysis.

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Day and night license plate detection using tail-light color and image features of license plate in driving road images

  • Kim, Lok-Young;Choi, Yeong-Woo
    • 한국컴퓨터정보학회논문지
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    • 제20권7호
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    • pp.25-32
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    • 2015
  • In this paper, we propose a license plate detection method of running cars in various road images. The proposed method first classifies the road image into day and night images to improve detection accuracy, and then the tail-light regions are detected by finding red color areas in RGB color space. The candidate regions of the license plate areas are detected by using symmetrical property, size, width and variance of the tail-light regions, and to find the license plate areas of the various sizes the morphological operations with adaptive size structuring elements are applied. Finally, the plate area is verified and confirmed with the geometrical and image features of the license plate areas. The proposed method was tested with the various road images and the detection rates (precisions) of 84.2% of day images and 87.4% of night images were achieved.

차량용 블랙박스 영상을 이용한 주간 신호등 탐지 및 인식 시스템 (Traffic Lights Detection and Recognition System Using Black-Box Images)

  • 황지은;안다솔;이승화;박성호;박천수
    • 반도체디스플레이기술학회지
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    • 제15권2호
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    • pp.43-48
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    • 2016
  • In this paper, we propose a traffic light detection and recognition (TLDR) algorithm in the daytime. The proposed algorithm utilizes the color and shape information for the TLDR. At first, a traffic light is detected and recognized based on its shape information. Then, the color range of the detected traffic light is investigated in HSV color space. The input data of the proposed TLDR algorithm is the color image captured using the black box camera during driving. Our simulations demonstrate that the proposed algorithm can achieve a high detection and recognition performance for the images including traffic lights.

소형 고체 레이저용 $NdAl_3(BO_3)_4$ 단결정 육성 (Growth of $NdAl_3(BO_3)_4$ Single Crystal for Miniature Solid State Laser)

  • 정선태;강진기;김정환;정수진
    • 한국세라믹학회지
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    • 제30권8호
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    • pp.643-650
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    • 1993
  • NdAl3(BO3)4 have been developed for miniature solid state laser material. Single crystals of NdAl3(BO3)4 were grown by TSSG technique using BaB4O7 flux. The effects of growth conditions such as cooling rate, seed orientation and rotation speed on crystal quality and the morphology were studied. At the cooling rate of 2.4$^{\circ}C$/day and the crystal rotation speed of 30~40rpm with the seed orientation in <201> or <100> directions, transparent and light violet colored crystals in size of 10$\times$15$\times$20㎣ with well developed {010}, {111}, {111}, {021}, {001}, {102}, {112}, {021} faces were obtained. By X-ray diffraction analysis, the space group was determined as C2/c, and the X-ray powder data was obtained.

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A study of a tidally interacting BCD pair, ESO 435-IG20 and ESO 435-IG16

  • Kim, Jinhyub;Sung, Eon-Chang;Chung, Aeree
    • 천문학회보
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    • 제39권1호
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    • pp.44.1-44.1
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    • 2014
  • Blue Compact Dwarf galaxies (BCDs) are systems that recently have experienced the burst of star formation. As one of the causes for active star formation in BCDs, tidal interaction (fly-by or merger) has been suggested. A pair of BCDs, ESO 435-IG20 and ESO 435-IG16 are separated by only ~80 kpc in projection at a similar redshift (at a ~9 Mpc distance), and hence suspected to be a good example of such case. Intergalactic atomic hydrogen gas found in HIPASS survey is also suggestive of this hypothesis. In this study, we probe the HI morphology and kinematics of this BCD pair using ATCA HI data to study detailed interaction history. We investigate various star formation tracers of the pair to study how responsible tidal interaction is for triggering star formation in these galaxies.

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Enhanced Control of OLED Deposition Processes by OVPD(R)

  • Schwambera, M.;Meyer, N.;Keiper, D.;Heuken, M.;Hartmann, S.;Kowalsky, W.;Farahzadi, A.;Niyamakom, P.;Beigmohamadi, M.;Wuttig, M.
    • 한국정보디스플레이학회:학술대회논문집
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    • 한국정보디스플레이학회 2007년도 7th International Meeting on Information Display 제7권1호
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    • pp.336-339
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    • 2007
  • The enhanced control of OLED deposition processes by Organic Vapor Phase Deposition $(OVPD^{(R)})$ is discussed. $OVPD^{(R)}$ opens a wide space of process control parameters. It allows the accurate and individual control of deposition layer properties like morphology and precise mixing of multi component layers (co-deposition) in comparison to conventional deposition manufacturing processes like e. g. VTE (vacuum thermal evaporation).

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HOST GALAXY OF TIDAL DISRUPTION OBJECT, SWIFT J1644+57

  • YOON, YONGMIN;IM, MYUNGSHIN;LEE, SEONG-KOOK;PAK, SOOJONG
    • 천문학논총
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    • 제30권2호
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    • pp.475-476
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    • 2015
  • We analyze the host galaxy of the tidal disruption object, Swift J1644+57, based on long-term optical to NIR data obtained with CQUEAN and UKIRT WFCAM observations. We decompose the bulge component using high resolution HST WFC3 images. We conclude that the host galaxy is bulge dominant. We investigate optical to NIR light curves and estimate the multi-band fluxes of the host galaxy. We fit spectral energy distribution (SED) models in order to determine the stellar mass. Finally, we estimate the mass of the black hole in the center of the host galaxy based on several scale relations.