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능동 발진 안테나를 이용한 소형 도플러 센서 (Compact Doppler Sensor Using Oscillator Type Active Antenna)

  • 윤기호
    • 전기전자학회논문지
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    • 제15권1호
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    • pp.49-56
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    • 2011
  • 본 논문에서는 고주파 발진회로의 공진기를 패치 안테나로 사용하는 능동발진 안테나를 2.4GHz 대역에서 제안하여 소형 무선도플러 센서로서 이동체의 거리나 속도 등을 측정할 수 있게 하였다. 이동체의 움직임은 고주파 발진 주파수의 천이를 발생시키며 이를 검출하는 회로를 통해 제안된 구조의 동작을 확인하였다. 설계 제작된 무선 도플러 센서는 직경이 30mm, 높이 4.2mm 정도로 매우 작은 원형디스크 형태를 갖으며, 안테나는 2.373GHz에서 약 130도의 빔폭과 전방향 방사특성을 나타내었다. 센서의 감도 측정결과, 1m 떨어져 움직이고 있는 도체판에 대해 최소 190mV의 도플러 신호 전압을 얻었고, 센서의 자유낙하 실험으로부터 지표상의 4.5m 지점에서 부터 지표면까지 전압크기가 선형적으로 증가하였다.

능동안테나의 발진주파수 편이에 의한 소형 거리 센서 (Compact Range Detection Sensor by Oscillation Frequency Deviation of an Active Antenna)

  • 윤기호
    • 한국정보통신학회논문지
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    • 제15권3호
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    • pp.528-535
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    • 2011
  • 본 논문에서는 고주파 발진회로의 공진기가 안테나로 동작하는 2.4GHz 대역의 능동 안테나를 이용하여 이동체의 거리를 측정할 수 있는 소형 도플러 센서를 제안하였다. 이동체의 움직임에 비례하여 고주파 발진주파수의 편이를 발생시키며 이를 검출하는 회로를 통해 제안된 구조의 동작을 확인하였다. 설계 제작된 거리 감지 센서는 직경이 30mm, 높이 4.2mm 정도로 매우 작은 원형디스크 형태를 갖으며, 안테나는 2.35GHz에서 약 120도의 빔폭과 전방향 방사특성을 나타내었다. 센서의 감도 측정결과, 1m 떨어져 움직이고 있는 도체판에 대해 약 240mV의 도플러 신호 전압을 얻었고, 자유낙하 실험으로부터 지표위의 5m 지점에서부터 지표면까지 선형적인 전압크기의 증가를 보였다.

돔 유리를 이용한 위치이동 다중화 홀로그램 정보저장장치용 서보 컨트롤 (Servo control for shift-multiplexed holographic data storage by using a dome-type glass)

  • 김성필;송석호;오차환;김필수;김지덕;이홍석
    • 한국광학회지
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    • 제15권1호
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    • pp.74-78
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    • 2004
  • 위치이동 다중화 홀로그램 정보저장장치에서, 돔 형태(dome-type)유리를 이용한 서보 컨트롤 방법을 제안하였다. 5개의 2차원 데이터를 재생효율 균일도 5% 이내로 위치이동 다중화 기록을 한 후, 직경이 25.4 mm 이고 두께가 1 mm 인 돔 유리를 사용하여, 재생 시에 발생하는 홀로그램 디스크의 기울어짐 각도오차가 $\pm$0.2$^{\circ}$,위치오차 $\pm$50$\mu\textrm{m}$인 경우에 대해서도 정확한 오차보정이 가능함을 실험적으로 검증하였다. 돔 유리를 이용하는 방식은 기존에 제안된 평판유리를 이용하는 방식[김성필 외, 한국광학회지, Vol. 14, No.1, pp. 58-64, 2003]에 비해 구동이 간편하기 때문에, 서보 컨트롤을 위한 광 픽업 장치를 간단하고 작은 규모로 모듈화 하는데 매우 유용하다.

TOWARD A NEXT GENERATION SOLAR CORONAGRAPH: DIFFRACTED LIGHT SIMULATION AND TEST RESULTS FOR A CONE OCCULTER WITH TAPERED SURFACE

  • Yang, Heesu;Bong, Su-Chan;Cho, Kyung-Suk;Choi, Seonghwan;Park, Jongyeob;Kim, Jihun;Baek, Ji-Hye;Nah, Jakyoung;Sun, Mingzhe;Gong, Qian
    • 천문학회지
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    • 제51권2호
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    • pp.27-36
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    • 2018
  • In a solar coronagraph, the most important component is an occulter to block the direct light from the disk of the sun. Because the intensity of the solar outer corona is $10^{-6}$ to $10^{-10}$ times of that of the solar disk ($I_{\odot}$), it is necessary to minimize scattering at the optical elements and diffraction at the occulter. Using a Fourier optic simulation and a stray light test, we investigated the performance of a compact coronagraph that uses an external truncated-cone occulter without an internal occulter and Lyot stop. In the simulation, the diffracted light was minimized to the order of $7.6{\times}10^{-10}I_{\odot}$ when the cone angle ${\theta}_c$ was about $0.39^{\circ}$. The performance of the cone occulter was then tested by experiment. The level of the diffracted light reached the order of $6{\times}10^{-9}I_{\odot}$ at ${\theta}_c=0.40^{\circ}$. This is sufficient to observe the outer corona without additional optical elements such as a Lyot stop or inner occulter. We also found the manufacturing tolerance of the cone angle to be $0.05^{\circ}$, the lateral alignment tolerance was $45{\mu}m$, and the angular alignment tolerance was $0.043^{\circ}$. Our results suggest that the physical size of coronagraphs can be shortened significantly by using a cone occulter.

$\cdot$ 영 동시조음 데이터베이스의 구축 (Speech Coarticulation Database of Korean and English)

  • 김종미
    • 한국음향학회지
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    • 제18권3호
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    • pp.17-26
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    • 1999
  • We present the first speech coarticulation database of Korean, English and Konglish/sup 3)/ named "SORIDA"/sup 4)/, which is designed to cover the maximum number of representations of coarticulation in these languages [1]. SORIDA features a compact database which is designed to contain a maximum number of triphones in a minimum number of prompts. SORIDA contains all consonantal triphones and vowel allophones in 682 Korean prompts of word length and in 717 English prompt words, spoken five times by speakers of balanced genders, dialects and ages. Korean prompts are synthesized lexicons which maximize their coarticulation variation disregarding any stress phenomena, while English prompts are natural words that fully reflect their stress effects with respect to the coarticulation variation. The prompts are designed differently because English phonology has stress while Korean does not. An intermediate language, Konglish has also been modeled by two Korean speakers reading 717 English prompt words. Recording was done in a controlled laboratory environment with an AKG Model C-100 microphone and a Fostex D-5 digital-audio-tape (DAT) recorder. The total recording time lasted four hours. SORIDA CD-ROM is available in one disk of 22.05 kHz sampling rate with a 16 bit sample size. SORIDA digital audio-tapes are available in four 124-minute-tapes of 48 kHz sampling rate. SORIDA′s list of phonetically-rich-words is also available in English and Korean.

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전산화단층 촬영상의 임계치가 3차원 의학모델 정확도에 미치는 영향에 대한 연구 (Influence of threshold value of computed tomography on the accuracy of 3-dimensional medical model)

  • 이병도;이완
    • Imaging Science in Dentistry
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    • 제32권1호
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    • pp.27-33
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    • 2002
  • Purpose: To evaluate the influence of threshold value of computed tomography on the accuracy of rapid prototyping (RP) medical model Material and Methods : CT datas of a human dry skull were transferred from CT scanner via compact disk to a personal computer (PC). 3-dimensional image reconstruction on PC by V-works/sup TM/ 3.0 (CyberMed. Inc.) software and RP models fabrication were followed. 2-RP models were produced by threshold value of 500 and 800 selected in surface rendering process. Linear measurements between arbitrary 12 anatomical landmarks on dry skull, 3-D image model, and 2-RP models were done and compared. Thus, the accuracy of 500 RP and 800RP models was respectively evaluated. Results: There was mean difference (% difference) in absolute value of 2.27 mm (2.73%) between linear measurements of dry skull and 500 RP model. There was mean difference (% difference) in absolute value of 1.94 mm (2.52%) between linear measurements of dry skull and 800 RP model. Conclusion: Slight difference of threshold value in rendering process of 3-D modelling made a influence on the accuracy of RP medical model.

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통전가압 소결된 Co-Fe, Co-Ni 소결체의 미끄럼 마찰 및 마멸거동 (Sliding Wear and Friction Behavior of Electro-Pressure Sintered Co-Fe and Co-Ni Compacts)

  • 권용진;김태웅;김용석
    • 한국분말재료학회지
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    • 제11권6호
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    • pp.451-461
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    • 2004
  • Dry sliding wear behavior of electro-pressure sintered Co-Fe and Co-Ni compacts was investigated. Pin-on-disk wear tests were performed on the sintered Co-Fe, Co-Ni disks against alumina $(Al_2O_3)$ and silica $(SiO_2)$ balls at various loads ranging from 3N to 12N. A constant sliding speed of 0.1m/sec was employed. Wear rate was calculated by dividing the weight loss of a specimen by the measured specific gravity and sliding dis-tance. Worn surfaces and cross-sections of the specimens were examined using an SEM and EDS to investigate wear mechanism of the compacts. The wear behavior of the compacts were discussed as a function of their com-position. Effects of mechancial properties of the compact as well as oxide layers formed on wearing surface on the wear were also discussed.

Raman O VI Profile Analysis of Accretion and Bipoloar Outflow in Sanduleak's Star

  • Heo, Jeong-Eun;Angeloni, Rodolfo;Di Mille, Francesco;Palma, Tali;Lee, Hee-Won
    • 천문학회보
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    • 제42권1호
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    • pp.58.4-59
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    • 2017
  • Sanduleak's star is a suspected symbiotic binary located in the Large Magellanic Cloud. It is known that it has a giant jet with physical size ~ 14pc. Its spectrum shows two strong emission bands at $6825{\AA}$ and $7082{\AA}$, which are originated from Raman-scattering of O VI by neutral hydrogen atoms. We present the high-resolution spectrum of Sanudleak's star obtained with MIKE at the Magellan-Caly telescope to investigate the O VI emission region based on the profiles of the two Raman features. In this spectrum, it is noted that the Raman $6825{\AA}$ feature exhibits a single broad peak profile, which is in high contrast with a clear triple peak profile of the Raman $7082{\AA}$ feature. In our analysis we suggest that the O VI emission region consist of three main emission parts: an accretion disk, a bipolar outflow and an optically thick, compact component surrounding the white dwarf. By performing Monte Carlo simulation we constrain the representative column density of the H I scattering region N_HI ~1${\times}$10^23 cm^-2, which is in accordance with the observed flux ratio in the two Raman features F(6825)/F(7082) ~ 4.5.

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Dispersal of Molecular Clouds by UV Radiation Feedback from Massive Stars

  • 김정규;김웅태
    • 천문학회보
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    • 제42권1호
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    • pp.38.1-38.1
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    • 2017
  • We report the results of three-dimensional radiation hydrodynamic simulations of star cluster formation in turbulent molecular clouds, with primary attention to how stellar radiation feedback controls the lifetime and net star formation efficiency (SFE) of their natal clouds. We examine the combined effects of photoionization and radiation pressure for a wide range of cloud masses (10^4 - 10^6 Msun) and radii (2 - 80 pc). In all simulations, stars form in densest regions of filaments until feedback becomes strong enough to clear the remaining gas out of the system. We find that the SFE is primarily a function of the initial cloud surface density, Sigma, (SFE increasing from ~7% to ~50% as Sigma increases from ~30 Msun/pc^2 to ~10^3 Msun/pc^2), with weak dependence on the initial cloud mass. Control runs with the same initial conditions but without either radiation pressure or photoionization show that photoionization is the dominant feedback mechanism for clouds typical in normal disk galaxies, while they are equally important for more dense, compact clouds. For low-Sigma clouds, more than 80% of the initial cloud mass is lost by photoevaporation flows off the surface of dense clumps. The cloud becomes unbound within ~0.5-2.5 initial free-fall times after the first star-formation event, implying that cloud dispersal is rapid once massive star formation takes place. We briefly discuss implications and limitations of our work in relation to observations.

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효율적인 복합다양체 CAD 시스템 위상 작업자 구현 (Implementation of Topological Operators for the Effective Non-manifold CAD System)

  • 최국헌
    • 한국공작기계학회:학술대회논문집
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    • 한국공작기계학회 2004년도 추계학술대회 논문집
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    • pp.382-387
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    • 2004
  • As the increasing needs in the industrial filed, many studies for the 3D CAD system are carried out. There are two types of 3D CAD system. One is manifold modeler, the other is non-manifold modeler. In the manifold modeler only 3D objects can be modeled. In the non-manifold modeler 3D, 2D, 1D, and 0D objects can be modeled in a unified data structure. Recently there are many studies on the non-manifold modeler. Most of them are focused on finding unknown topological entities and representing all kinds of topological entities found. In this paper, efficient data structure is selected. The boundary information on a face and an edge is included in this data structure. The boundary information on a vertex is excluded considering the frequency of usage. Because the disk cycle information is not required in most case of modeling. It is compact. It stores essential non-manifold information such as loop cycle and radial cycle. A suitable Euler-Poincare equation is studied and selected. Using the efficient data structure and the selected Euler-Poincare equation, 18 basic Euler operators are implemented. Several 3D models are created using the implemented modeler. A non-manifold modeling can be carried out using the implemented 3D CAD system. The results of this paper could be used in the further studies such as an implementation of Boolean operators, and a translation of 2D CAD drawings to 3D models.

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