• 제목/요약/키워드: Space Matching

검색결과 492건 처리시간 0.022초

A Study on Blended Inlet Body Design for a High Supersonic Unmanned Aerial Vehicle

  • You, Lianxing;Yu, Xiongqing;Li, Hongmei
    • International Journal of Aeronautical and Space Sciences
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    • 제17권2호
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    • pp.260-267
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    • 2016
  • The design process of blended inlet body (BIB) for the preliminary design of a near-space high supersonic unmanned aerial vehicle (HSUAV) is presented. The mass flow rate and cowl area of inlet at a design point are obtained according to the cruise condition of the HSUAV. A mixed-compression axisymmetric supersonic inlet section with a fixed geometry reasonably matching the high supersonic cruise state is created by using the inviscid theory of aerodynamics. The inlet section is optimized and used as a baseline section for the BIB design. Three BIB concepts for the HSUAV are proposed, and their internal aerodynamic characteristics of inlet are evaluated using Euler computational fluid dynamics (Euler CFD) solver. The preferred concept is identified, in which the straight leading edge of the baseline HSUAV configuration is modified into the convex leading edge to accommodate the inlet and meet the requirements of the cowl area to capture the sufficient air flow. The total recovery of inlet for the preferred BIB concept and the aerodynamic characteristics of the modified HSUAV configuration are verified using Navier-Stokes computational fluid dynamics (NS CFD) solver. The validation indicates that the preferred BIB concept can meet both the requirements of the inlet and aerodynamic performance of the HSUAV.

공공아파트 건설공사의 공간별 공사비분류체계 개발 (Development of the Space Cost Breakdown Structure(CBS) for Multi-Family Housing Projects)

  • 현창택;구교진;연희정;문현석;조규만;홍태훈
    • 한국건설관리학회논문집
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    • 제8권6호
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    • pp.178-187
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    • 2007
  • 최근 정부의 주택보급정책 강화에 따라 공공아파트 건설공사의 건축공사비에 대한 관심이 높아지고 있다. 그러나 현재 공공아파트 공사비내역 구성은 공종별 분류체계로 구성되어 있어, 공공아파트의 건축공사비를 체계적으로 예측하는 것은 현실적으로 많은 문제점을 지니고 있다. 이에 본 연구에서는 공공아파트 프로젝트 기획 및 설계단계에서 좀 더 합리적인 공사비 예측을 위해, 델파이분석(Delphi)기법을 이용하여 공공아파트 공간별 공사비분류체계를 개발하였다. 공공아파트 공간별 공사비분류체계는 공공아파트의 공간별 특성을 반영하여 주택부문, 주택외부문, 가산부문 등으로 구분하였으며, 각각의 부문을 공간별 해당 부위와 각 세부공종으로 세분화하였다. 또한 구축된 공간별 공사비분류체계에 공공아파트 공사비 내역서를 분석하여 공간별 분류체계의 실용성 및 유효성을 검증하였다.

Utility of False Profile View for Screening of Ischiofemoral Impingement

  • Kwak, Dae-Kyung;Yang, Ick-Hwan;Kim, Sungjun;Lee, Sang-Chul;Park, Kwan-Kyu;Lee, Woo-Suk
    • Hip & pelvis
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    • 제30권4호
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    • pp.219-225
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    • 2018
  • Purpose: Ischiofemoral impingement (IFI)-primarily diagnosed by magnetic resonance imaging (MRI)-is an easily overlooked disease due to its low incidence. The purpose of this study was to evaluate the usefulness of false profile view as a screening test for IFI. Materials and Methods: Fifty-eight patients diagnosed with IFI between June 2013 and July 2017 were enrolled in this retrospective study. A control group (n=58) with matching propensity scores (age, gender, and body mass index) were also included. Ischiofemoral space (IFS) was measured as the shortest distance between the lateral cortex of the ischium and the medial cortex of lesser trochanter in weight bearing hip anteroposterior (AP) view and false profile view. MRI was used to measure IFS and quadratus femoris space (QFS). The receiver operating characteristics (ROC), area under the ROC curve (AUC) and cutoff point of the IFS were measured by false profile images, and the correlation between the IFS and QFS was analyzed using the MRI scans. Results: In the false profile view and hip AP view, patients with IFI had significantly decreased IFS (P<0.01). In the false profile view, ROC AUC (0.967) was higher than in the hip AP view (0.841). Cutoff value for differential diagnosis of IFI in the false profile view was 10.3 mm (sensitivity, 88.2%; specificity, 88.4%). IFS correlated with IFS (r=0.744) QFS (0.740) in MRI and IFS (0.621) in hip AP view (P<0.01). Conclusion: IFS on false profile view can be used as a screening tool for potential IFI.

가상현실과 실공간 동기화를 위한 공간 위치보정 측정 방법론에 대한 연구 (A Study on the Measurement Method of Spatial Position Compensation for Virtual Reality and Real Space Synchronization)

  • 박기진;이병학;김남혁;윤성호
    • 한국기계가공학회지
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    • 제17권6호
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    • pp.136-143
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    • 2018
  • Recently, with the rapid development of virtual reality technology, there have been more and more applications of virtual reality technology in various fields. In order to realize a virtual reality, a method of implementing a visualization environment through an HMD (Head Mounted Display) is widely used. However, in the current visualization environment through the HMD, the user feels dizziness when worn, It has the disadvantage of imposing restrictions on. In this study, it is aimed to realize virtual reality visualization environment through multi-screen environment which improves the experience effect of virtual environment by using existing screen instead of visualization through HMD, and compensates for shortcomings of HMD method. In order to realize a multi-screen environment as a highly visualized environment, a technique for matching the spatial position of the multi-screen with the spatial position of the virtual environment is required. To do this, we need an efficient method to precisely measure the position of the space, and we propose a spatial position compensation methodology that can efficiently and precisely measure the position of the real space and reflect it in the virtual environment.

Design Optimization of Composite Radar Absorbing Structures to Improve Stealth Performance

  • Jang, Byungwook;Kim, Myungjun;Park, Jungsun;Lee, Sooyong
    • International Journal of Aeronautical and Space Sciences
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    • 제17권1호
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    • pp.20-28
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    • 2016
  • In this study, an efficient method of designing laminate composite radar absorbing structures (RAS) is proposed with consideration given to the structural shape so as to improve aircraft stealth performance. The calculation of the radar cross section (RCS) should be decreased to enhance the efficiency of the stochastic optimization when designing an RAS. In the proposed method, RAS are optimized to match up the input impedance of the minimal RCS, which is obtained by using physical optics and the transmission line theory. Single and double layer dielectric RAS for aircraft wings are employed as numerical examples and designed using the proposed method, RCS minimization and reflection coefficient minimization. The availability of the proposed method is assessed by comparing the similarity of the results and computation time with other design methods. According to the results, the proposed method produces the same results as the stochastic optimization, which adopts the RCS as the objective function, and can improve RAS design efficiency by reducing the number of RCS analyses.

스케일 공간 도함수를 이용한 강인한 기술자 생성 기법 (A Method of Constructing Robust Descriptors Using Scale Space Derivatives)

  • 박종승;박운상
    • 정보과학회 논문지
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    • 제42권6호
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    • pp.764-768
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    • 2015
  • 멀티미디어 데이터의 생산과 소비가 증가함에 따라 이를 효과적으로 처리하고 관리하는 데 필요한 이미지 검색 기술의 필요성이 점차 커지고 있다. 본 논문에서는 이미지 검색 기법 중 최근 주목 받고 있는 특징점 기반의 이미지 검색 방법에서 기존 보다 강인한 기술자를 생성하는 방법을 제안한다. 즉, 스케일 공간 이미지에 더하여 1차 및 2차 미분 이미지를 기술자 생성에 이용함으로써 기술자의 변별력을 향상시키도록 한다. 제시되는 기술자는 다양한 영상 변환을 포함하는 공용 데이터 셋을 이용하여 성능 평가를 수행하였다. 새로운 기술자는 길이가 약간 증가하는 단점이 있으나 특징점 매칭에 있어서 현저한 성능 향상을 보인다.

비선형 추종제어를 위한 성층권비행선의 궤적 최적화 (Trajectory Optimization for Nonlinear Tracking Control in Stratospheric Airship Platform)

  • 이상종;방효충;장재원;성기정
    • 한국항공우주학회지
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    • 제37권1호
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    • pp.42-54
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    • 2009
  • 비행체의 최적궤적문제에서는 최적화의 수렴성 및 효율성을 위해 3자유도 운동역학모델이 이용되며, 비선형 추종제어를 위해서는 6자유도 비선형 운동모델이 이용된다. 따라서, 3자유도 운동역학모델을 통해 획득한 최적궤적을 비선형 추종제어의 기준궤적으로 사용하는 경우에 두 모델간의 상이성으로 인한 문제가 발생하게 되며 성능이 보장하지 못한다. 본 논문에서는 이러한 두 모델간의 차이를 완화시키기 위한 새로운 최적궤적 생성 방법을 제안하였으며, 성층권비행선의 실제 구속조건과 성능조건 및 제트 스트림을 고려하여 최적궤적을 생성하고 기존 결과와 비교함으로써 제안한 방법의 장점을 검증하였다.

정밀 행성 착륙을 위한 지형 보조 관성 항법 연구 (Terrain Aided Inertial Navigation for Precise Planetary Landing)

  • 정보영;최윤혁;조수장;방효충
    • 한국항공우주학회지
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    • 제38권7호
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    • pp.673-683
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    • 2010
  • 본 논문에서는 정밀 행성 착륙을 위해 광학센서와 관성항법시스템을 이용한 지형보조 관성항법 시스템을 구현하였다. 또한 측정된 지형 데이터와 사전에 탑재한 지형 데이터간의 특징점 추출, 매칭, 추적의 영상 처리 과정을 수행하였고 이를 통해 특징점의 좌표를 추출할 수 있다. 반복 확장칼만필터를 이용한 항법 시스템은 기존 관성 항법 장치의 항법 오차 누적을 보상하여 보다 정밀한 항법 정보를 제공한다. 이는 향후 착륙선의 유도 및 제어 법칙과 결합하여 정밀 행성 착륙을 위한 시스템 구현에 적용이 가능하다.

Wide band prototype feedhorn design for ASTE focal plane array

  • Lee, Bangwon;Gonzales, Alvaro;Lee, Jung-won
    • 천문학회보
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    • 제41권2호
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    • pp.66.2-66.2
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    • 2016
  • KASI and NAOJ are making collaborating efforts to implement faster mapping capability into the new 275-500 GHz Atacama Submillimeter Telescope Experiment focal plane array (FPA). Feed horn antenna is one of critical parts of the FPA. Required fractional bandwidth is almost 60 % while that of traditional conical horn is less than 50 %. Therefore, to achieve this wideband performance, we adopted a horn of which the corrugation depths have a longitudinal profile. A profiled horn has features not only of wide bandwidth but also of shorter length compared to a linear-tapered corrugated horn, and lower cost fabrication with less error can be feasible. In our design process the flare region is represented by a cubic splined curve with several parameters. Parameters of the flare region and each dimension of the throat region are optimized by a differential evolution algorithm to keep >20 dB return loss and >30 dB maximum cross-polarization level over the operation bandwidth. To evaluate RF performance of the horn generated by the optimizer, we used a commercial mode matching software, WASP-NET. Also, Gaussian beam (GB) masks to far fields were applied to give better GB behavior over frequencies. The optimized design shows >23 dB return loss and >33 dB maximum cross-polarization level over the whole band. Gaussicity of the horn is over 96.6 %. The length of the horn is 12.5 mm which is just 57 % of the ALMA band 8 feed horn (21.96 mm).

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Estimation of Halo CME's radial speeds using coronal shock waves based on EUV observations

  • Jeong, Hyunjin;Moon, Yong-Jae
    • 천문학회보
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    • 제43권1호
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    • pp.54.4-55
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    • 2018
  • Propagating speeds of coronal mass ejections (CMEs) have been calculated by several geometrical models based on multi-view observations (STEREO/SECCHI and SOHO/LASCO). But in 2015, we were unable to obtain radial velocity of a CME because the STEREO satellites were located near the backside of the sun. As an alternative to resolve this problem, we propose a method to combine a coronal shock front, which appears on the outermost of the CME, and an EUV-wave that occurs on the solar disk. According to recent studies, EUV-wave occurs as a footprint of the coronal shockwave on the lower solar atmosphere. In this study, the shock, observed as a bubble shape, is assumed as a perfect sphere. This assumption makes it possible to determine the height of a coronal shock, by matching the position of an EUV-wave on the solar disk and a coronal shock front in coronagraph. The radial velocity of Halo-CME is calculated from the rate of coronal shock position shift. For an event happened on 2011 February 15, the calculated speed in this method is a little slower than the real velocity but faster than the apparent one. And these results and the efficiency of this approach are discussed.

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