• 제목/요약/키워드: Space scan

검색결과 261건 처리시간 0.027초

하악대구치의 치성감염으로 유발된 안와골막하농양의 치험례 (ORBITAL SUBPERIOSTEAL ABSCESS SECONDARY TO ODONTOGENIC INFECTION OF LOWER MOLAR : A CASE REPORT)

  • 김동률;홍광진;최동주;이정구
    • Maxillofacial Plastic and Reconstructive Surgery
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    • 제22권1호
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    • pp.110-116
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    • 2000
  • A 61-years old man with diabetes mellitus(DM) was admitted to our hospital, complaining of progressive right periorbital swelling, headache and toothache on the right lower second molar. On the first visit, moderate swelling was noticed from the right periorbital region with exophthalmos and subconjunctival effusion. Intraorally, right lower second molar had a severe periodontal disease and fistular formation on its distal area. From 3 days after hospitalization, the visual acuity of his right eye was gradually worsen and we performed CT scan. CT scan demonstrated an inflammatory change at the right orbit with subperiosteal abscess at the inferior orbital wall, which was extended from the right infratemporal, parapharyngeal and internal pterygoid space. Patient was treated by mean of intraoral(right upper vestibular and retromolar) and extraoral(infraorbital) incision and drainage, massive anti-therapy and DM control. The patient improved gradually and finally was discharged from the hospital, but his visual loss of right side was not recovered.

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로젯 주사 적외선 탐색기의 순시 시계 설계에 관한 연구 (A study on design of instantaneous field of view of rosette scanning infrared seeker)

  • 장성갑;홍현기;한성현;최종수
    • 전자공학회논문지S
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    • 제35S권7호
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    • pp.86-94
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    • 1998
  • The rosette-scan seeker is a device mounted on the infrared guided missile. It offers the positions and iamges of target to missiles servo system by scanning a space about target in rosette pattern with a single detector. An instantaneous field of view (IFOV), which is a diameter of a detector moving along the path of the rosette pattern, has the property that its smaller size provide the less interference of background signals and detector noise. If its size is too small to voer the total field of view (TFOV), however, it produces the invisible regions in the TFOV. In this case, the invisible regions cause the performance of the seeker to deteriorate. For full scan-coverage, it is necessary to design the small IFOV without the invisible regions in the TFOV, as possible. In this paper, we propose the new method of designing the smaller IFOV than the conventional method and verify full coverage of the scanned region. By comparing the nose equivalent flux density (NEFD) of the proposed method with the that of the conventional one, we confirm that the former is better than the latter in terms of performance.

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ADVANTAGES OF THE AKARI FIR ALL-SKY MAPS

  • Doi, Yasuo;Takita, Satoshi;Ootsubo, Takafumi;Arimatsu, Ko;Tanaka, Masahiro;Morishima, Takahiro;Kawada, Mitsunobu;Matsuura, Shuji;Kitamura, Yoshimi;Hattori, Makoto;Nakagawa, Takao;White, Glenn;Ikeda, Norio
    • 천문학논총
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    • 제32권1호
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    • pp.11-15
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    • 2017
  • We present the AKARI far-infrared (FIR) all-sky maps and describe its characteristics, calibration accuracy and scientific capabilities. The AKARI FIR survey has covered 97% of the whole sky in four photometric bands, which cover continuously 50-180 micron with band central wavelengths of 65, 90, 140, and 160 microns. The data have been publicly released in 2014 (Doi et al., 2015) with improved data quality that have been achieved since the last internal data release (Doi et al., 2012). The accuracy of the absolute intensity is ${\leq}10%$ for the brighter regions. Quantitative analysis of the relative intensity accuracy and its dependence upon spatial scan numbers has been carried out. The data for the first time reveal the whole sky distribution of interstellar matter with arcminute-scale spatial resolutions at the peak of dust continuum emission, enabling us to investigate large-scale distribution of interstellar medium in great detail. The filamentary structure covering the whole sky is well traced by the all-sky maps. We describe advantages of the AKARI FIR all-sky maps for the study of interstellar matter comparing to other observational data.

A Study on Optimized Mapping Environment for Real-time Spatial Mapping of HoloLens

  • Hwang, Leehwan;Lee, Jaehyun;Hafeez, Jahanzeb;Kang, Jinwook;Lee, Seunghyun;Kwon, Soonchul
    • International Journal of Internet, Broadcasting and Communication
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    • 제9권3호
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    • pp.1-8
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    • 2017
  • Recently, the development of the head mounted display (HMD) device has attracted a great deal of attention to the actual contents. Especially, Augmented Reality (AR), which is a mixture of actual information and virtual world information, is focused on. AR HMD is able to interact by arranging virtual objects in real space through spatial recognition using depth camera. In order to naturally mix virtual space with real space, it is necessary to develop a technology for realizing spatial mapping information with high accuracy. The purpose of this paper is to evaluate the optimal configuration of augmented reality application program by realizing accurate spatial mapping information when mapping a real space and an object placement environment using HoloLens. To do this, we changed the spatial mapping information in real space to three levels, which are the number of meshes used in cubic meters to scan step by step. After that, it was compared with the 3D model obtained by changing the actual space and mesh number. Experimental result shows that the higher the number of meshes used in cubic meters, the higher the accuracy between real space and spatial mapping. This paper is expected to be applied to augmented reality application programs that require scanning of highly mapped spatial mapping information.

1.6 m 신태양망원경용 고속영상태양분광기 개발 (DEVELOPMENT OF THE FAST IMAGING SOLAR SPECTROGRAPH FOR 1.6 m NEW SOLAR TELESCOPE)

  • 나자경;채종철;박영득;박형민;장비호;안광수;양희수;조경석;김연한;김광동
    • 천문학논총
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    • 제26권1호
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    • pp.45-54
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    • 2011
  • KASI and Seoul National University developed the Fast Imaging Solar Spectrograph (FISS) as one of major scientific instruments for the 1.6 m New Solar Telescope (NST) and installed it in the Coude room of the NST at Big Bear Solar Observatory (BBSO) in May, 2010. The major objective of the FISS is to study the fine-scale structures and dynamics of plasma in the photosphere and chromosphere. To achieve it, the FISS is required to take data with a spectral resolution higher than $10^5$ at the spectrograph mode and a temporal resolution less than 10 seconds at the imaging mode. The FISS is a spectrograph using Echelle grating and has characteristics that can observe dual bands (H${\alpha}$ and CaII 8542) simultaneously and perform fast imaging using fast raster scan and two fast CCD cameras. In this paper, we introduce briefly the whole process of FISS development from the requirement analysis to the first observations.

경추증성 척수증의 증상발현과 경미한 외상 사이의 관련성에 대한 의료감정 1례 (A Case of Medical Examination for the Relationship between Symptom onset of cervical spondylotic myelopathy and minor trauma)

  • 김상현
    • 보험의학회지
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    • 제27권2호
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    • pp.107-111
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    • 2008
  • The Cervical spondylotic myelopathy (CSM) is degenerative compressive myelopathy which initiation of symptoms seems to be induced by minor cervical trauma or spontaneous event. There was a case of Claim medical examination which was requested to discriminate the cause of ambulatory quadriparesis. Patient asserted that the onset of his myelopathy was followed by minor trauma. The author considered the medical recordings, MRI scan, Claim reports by claim manager. The space available for cord was the smallest at C3-4 level. But on MRI findings, the spinal cord at C3-4 level seemed to be already damaged. There were no recent injury evidences such as hemorrhages, spinal cord contusions, edema, soft tissue hemorrhages. If the space available for cord was small enough to compress the spinal cord, the serious neurologic deficits, non-ambulatory quadriplegia, etc were commonly induced by cervical extension trauma. Patient's asserts did not correspond to his clinical course after cervical trauma. The author reports a case of medical examination for the relationship between symptom onset of cervical spondylotic myelopathy and minor trauma within author's experience.

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Synovial Chondromatosis in the Temporomandibular Joint: Report of Two Cases

  • 하용찬;김철환
    • 대한치과의사협회지
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    • 제55권10호
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    • pp.706-714
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    • 2017
  • Background Synocial chondromatosis(SC), a proliferative disorder of the synovial membrane. The etiology or cause of SC remains unclear. SC usually occurs in large articular joints such as knee, hip, elbow, and ankle. SC of the TMJ is very rare. It is a benign disease that mainly affects unilateral side. It can form cartilagenous and calcified loose bodies of various sizes and cause abnormal function of TMJ. Case Report In this paper, we report two cases of SC in the upper joint space of the left TMJ. One complained that "Sometimes the left jaw joint feels disoriented" and the other had no symptoms. CT scan and MRI showed left TMJ space widening, multiple tiny calcified mass. After clinical and radiographic analysis, we performed surgical removal of the lesion under genereal anesthesia. In the histologic examination, synovial chondromatosis was diagnosed in both patients. Conclusions We report two cases of synovial chondromatosis in the upper joint space of the left TMJ. We performed surgical removal of the lesion. The two patients showed good prognosis without recurrence or pain up to date.

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Search for Very Fast Variability in AGN Radio Light Curves

  • 이태석;;손봉원;이상성;변도영;오정환
    • 천문학회보
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    • 제38권1호
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    • pp.43.1-43.1
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    • 2013
  • We present here the preliminary results of the fast variability of AGN radio light curves. The shortest time scale of minute in AGN light curves is needed to probe the AGN activity for a few reasons; First, to check if there is any kind of shortest time scale activity. Secondly, to find out what high frequency end of AGN spectra look like. For the last, to see the time delay at several wavelength bands and the change of the spectral index with time. The observation was conducted with three KVN(Korea VLBI Network) antennas with single dish cross scan mode. In order not to lose the target at any given time, whenever one station needs to observe the calibrator, the other station is on the target. Though the detailed data reduction is still going on, there might exist varying feature in the radio light curve. The more fine calibration will be done in near future and another good data set is ready for the reduction.

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3D 스캔 분석을 통한 전통조경 계획 및 설계 활용방안 (A Measure of Landscape Planning and Design Application through 3D Scan Analysis)

  • 신현실
    • 한국전통조경학회지
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    • 제36권4호
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    • pp.105-112
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    • 2018
  • 본 연구는 조경계획 및 설계 분야에 3D 스캔기술을 적용하기 위한 연구로 전통조경공간 계획설계에 대한 디지털화 방안을 모색하고자 담양 소쇄원과 성락원을 대상으로 3D 스캔을 실시한 결과는 다음과 같다. 첫째, 3D 스캔을 통한 전통정원의 실측 결과 각 관측지점에서 취득한 점 데이터를 기반으로 좌표값의 병합, 데이터의 후처리 과정을 통해 ${\pm}3-5mm$ 오차의 정밀한 3차원의 모델링을 구축 되는 것을 확인하였다. 둘째, 3D 측량 결과 소쇄원의 경우는 제월당, 광풍각과 주변의 담장과 석축, 애양단 담장 등에 대한 측량 데이터를 얻었으며 성락원은 영벽지 일대의 지형과 바위각자, 송석정 일대의 암반부와 수로 주변에 대한 측량 데이터를 얻었다. 위의 자료들은 정원의 변화모습도 모니터링 할 수 있다는 장점이 있다. 셋째, 3D 스캔을 통해 구축된 공간정보는 정밀실측데이터를 포함하고 있는 3차원상의 도면 작성과 점검 툴을 구축할 수 있으며, 이러한 과정은 조경공간의 실측과 조사 과정에서 시간과 인력에 대한 경제성을 확보할 수 있었다. 또한 3차원상의 1:1 스케일을 지닌 모델링은 설계 규모에 따라 신뢰할만한 공간데이터가 유지된 채 특정 크기로 재가공할 수 있다는 점에서 효율성이 높을 것으로 기대된다. 이외에 장기적 관점에서 3D 스캔 데이터의 구축은 시간의 경과에 따른 전통조경공간의 변화를 예측하고 시뮬레이션 하는데 용이하다.

시차공간영상을 이용한 스테레오 영상 정합에 관한 연구 (A Study on Stereo Matching Algorithm using Disparity Space Image)

  • 이종민;김대현;최종수
    • 대한전자공학회논문지SP
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    • 제41권6호
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    • pp.9-18
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    • 2004
  • 본 논문에서 우리는 시차공간영상 (disparity space image)을 이용한 새로운 스테레오 정합 방법을 제안한다. 본 논문에서는 실측 제어점 대신 영상 안에서 특징점을 추출하여 정합영역을 설정하였고, 간단한 비용행렬을 정의하였다. 그리고 정합 속도를 증가시키기 위해 화소 단위의 정합을 이용하였다. 화소 단위의 정합은 정합 속도는 향상시키지만, 주변 영역을 이용하지 않기 때문에 정합의 정확성이 낮아진다. 이러한 단점을 보완하기 위해 시차공간영상의 특성을 이용하여 정합경로를 확대시켜서 주변 영역을 최대한 이용하였다. 또한, 현재 위치에서 이전과 이후의 시차공간영상을 체적화하여 전후의 시차공간영상을 이용함으로써 정합의 정확도를 더욱 향상시키는 정합 보정 모듈을 추가하였다. 본 논문에서 제안된 알고리즘은 다양한 영상에 적용하여 실험하였고, 그 결과 제안된 방법의 우수한 성능을 확인할 수 있었다.