• 제목/요약/키워드: Optical Height

검색결과 347건 처리시간 0.027초

Variations of Interface Potential Barrier Height and Leakage Current of (Ba, Sr)$TiO_3$ Thin Films Deposited by Sputtering Process

  • Hwang, Cheol-Seong;Lee, Byoung-Taek
    • The Korean Journal of Ceramics
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    • 제2권2호
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    • pp.95-101
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    • 1996
  • Variations of the leakage current behaviors and interface potential barrier $({\Phi}_B)$ of rf-sputter deposited (Ba, Sr)$TiO_3$ (BST) thin films with thicknesses ranging from 20 nm to 150nm are investigated as a function of the thickness and bias voltages. The top and bottom electrodes are dc-sputter-deposited Pt films. ${\Phi}_B$ critically depends on the BST film deposition temperature, postannealing atmosphere and time after the annealing. The postannealing under $N_2$ atmosphere results in a high interface potential barrier height and low leakage current. Maintaining the BST capacitor in air for a long time reduces the ${\Phi}_B$ from about 2.4 eV to 1.6 eV due to the oxidation. ${\Phi}_B$ is not so dependent on the film thickness in this experimental range. The leakage conduction mechanism is very dependent on the BST film thickness; the 20 nm thick film shows tunneling current, 30 and 40 nm thick films show Shottky emission current.

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수정된 화인 맵을 이용한 2-파장 홀로그래피와 잡음 제거 연구 (Study on Error Reduction in Dual Wavelength Digital Holography Using Modified Fine Map)

  • 유영훈
    • 한국광학회지
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    • 제22권3호
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    • pp.129-133
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    • 2011
  • 2-파장 홀로그래피에서 수정된 화인 맵을 이용하여 2-파장 홀로그래피에서 발생하는 잡음 증폭현상을 줄이는 연구를 수행하였다. 일반 적인 화인 맵은 측정체의 단차가 2-파장 홀로그래피에 사용되는 광원의 파장보다 작은 경우에는 잡음을 잘 줄일 수 있으나, 단차가 파장 보다 큰 경우에는 측정 결과에 영향을 주어 잘못 된 측정 결과를 보인다. 이러한 오차를 줄이기 위하여 수정된 화인 맵을 이용하였으며, 그 결과 측정체의 단차가 파장 보다 큰 경우에도 측정에 영향을 주지 않고 잡음을 줄일 수 있음을 확인 하였다.

Fabrication of Multi-layered Macroscopic Hydrogel Scaffold Composed of Multiple Components by Precise Control of UV Energy

  • Roh, Donghyeon;Choi, Woongsun;Kim, Junbeom;Yu, Hyun-Yong;Choi, Nakwon;Cho, Il-Joo
    • BioChip Journal
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    • 제12권4호
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    • pp.280-286
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    • 2018
  • Hydrogel scaffolds composed of multiple components are promising platform in tissue engineering as a transplantation materials or artificial organs. Here, we present a new fabrication method for implementing multi-layered macroscopic hydrogel scaffold composed of multiple components by controlling height of hydrogel layer through precise control of ultraviolet (UV) energy density. Through the repetition of the photolithography process with energy control, we can form several layers of hydrogel with different height. We characterized UV energy-dependent profiles with single-layered PEGDA posts photocrosslinked by the modular methodology and examined the optical effect on the fabrication of multi-layered, macroscopic hydrogel structure. Finally, we successfully demonstrated the potential applicability of our approach by fabricating various macroscopic hydrogel constructs composed of multiple hydrogel layers.

교육용 시스템 개발과 실시간 비선형 제어(II) (Development of an Educational System and Real Time Nonlinear Control (II))

  • 박성욱
    • 대한전기학회논문지:시스템및제어부문D
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    • 제51권12호
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    • pp.571-576
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    • 2002
  • This paper is to develop jumping ring system with three sensor arrays and to control levitated ring using dynamic neural mode. Placing an aluminum ring on the core and switching on an AC source causes the ring to jump in the air due to induced currents. The educational system is composed of 40th optical sensor array, encode circuit, 89C51 microprocessor and control board. The control board consists of power IC, and phase controller. Real time process is present to obtain a height of levitated ring for three different sensor arrays. Based on the educational system and the proposed dynamic neural mode, the height of levitation of the ring is controlled by reference signals. This paper focuses on real system controls using the dynamic neural mode with on line learning algorithm.

초음파의 에코 높이를 이용한 미소(微小) 박리(剝離) 두께 측정에 관한 연구 (Measurement of Infinitesimal Delaminaton Thickness by Echo Amplitude of Ultrasonic Wave)

  • 한응교;장경영;황병일;이범성;박익근
    • 비파괴검사학회지
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    • 제13권1호
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    • pp.21-28
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    • 1993
  • If the infinitesimal delamination exists and the two waves can hardly be distinguished from each other on account of being much closer, we cannot measure the thickness of delamination by the time difference method. On this study, we calculated the thickness of infinitesimal delamination model by means of measuring echo height due to the deflection of material particles and utilized Newton Ring for optical measurement as a delamination model. From the result of Newton Ring expressed in the delamination model, we can calculate the infinitesimal delamination thickness up to $0.2{\sim}0.3{\mu}m$ due to the difference of acoustic impedance by the ratio of the echo height to the total reflection.

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광산란 소멸법을 이용한 층류확산화염내에 매연입자의 크기 및 농도 측정 (Soot Size and Concentration Measurements in a Laminar Diffusion Flame Using a Lignt Scattering/Extinction Technique)

  • 하영철;김상수
    • 대한기계학회논문집
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    • 제16권9호
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    • pp.1796-1804
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    • 1992
  • 본 연구에서는 동심확산화염내에 생기는 매연 입자의 크기와 농도를 광산란 소멸법으로 보다 정확히 측정하여 궁극적 목적인 매연입자 제어의 기반을 조성하고자 한다.

태양열집속집열기의 설계 방법에 관한 연구 (A New Approach to Design Method of the Solar Compound Parabolic Concentrator with Tubular Absorber)

  • 김석종;임상훈
    • KIEAE Journal
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    • 제2권3호
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    • pp.33-38
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    • 2002
  • The intermediate range of temperatures($100{\sim}300^{\circ}C$) which can be achieved with CPCs(Compound Parabolic Concentrators) without tracking device provides both economic and thermal advantages for solar collector design. The present paper summarizes critical design considerations for CPC with cylindrical absorber and its optical performance using ray tracing program. Concentration ratios vary as acceptance half angle, ratio of reflector height to aperture width and ratio of reflector area to aperture area. This effects showed that the concentration ratio was increased as acceptance angle but optimum ratio of reflector height to aperture width existed at critical value. As a result of ray tracing, solar ray losses was maximized at acceptance half angle and this problem was solved by increasing absorber tube diameter. The concentrating flux distribution on the absorber surface was uniform but peak flux existed.

Analysis of Laser Control Effects for Direct Metal Deposition Process

  • Choi Joo-Hyun;Chang Yoon-Sang
    • Journal of Mechanical Science and Technology
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    • 제20권10호
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    • pp.1680-1690
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    • 2006
  • As a promising and novel manufacturing technology, laser aided direct metal deposition (DMD) process produces near-net-shape functional metal parts directly from 3-D CAD models by repeating laser cladding layer by layer. The key of the build-up mechanism is the effective control of powder delivery and laser power to be irradiated into the melt-pool. A feedback control system using two sets of optical height sensors is designed for monitoring the melt-pool and real-time control of deposition dimension. With the feedback height control system, the dimensions of part can be controlled within designed tolerance maintaining real time control of each layer thickness. Clad nugget shapes reveal that the feedback control can affect the nugget size and morphology of microstructure. The pore/void level can be controlled by utilizing pulsed-mode laser and proper design of deposition tool-path. With the present configuration of the control system, it is believed that more innovation of the DMD process is possible to the deposition of layers in 3-D slice.

빛 공해 방지를 위한 유럽형 LED 가로등용 비구면 광학계에 관한 연구 (A Study on Aspheric Optics European LED Streetlights Type for the Prevention of Light Pollution)

  • 이시우;이창수;현동훈
    • 한국생산제조학회지
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    • 제22권3호
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    • pp.429-436
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    • 2013
  • In this study, we researched a pendant-type aspherical optical system, which could be applied to street lighting and security lighting in Europe. The goal of this research was eco-friendly artificial lighting that could be used for the one-to-one replacement of ordinary lighting. LED lighting was miniaturized by using one COB LED Module and one aspherical optical system, which could control the luminosity of the LED. Through the aspherical optical system, the light distribution angle could be controlled in a range of $140^{\circ}$ for the X-axis and $40^{\circ}$ for the Y-axis. This means that this optical system is appropriate for catenary-type lighting, which is widely used in Europe on both narrow and broad roads. The performance was determined using a lighting simulation program. This lighting system simulation showed that road rates M4 and M5 could be satisfied, with the condition of a 13-m height and 50-m distance (U0 and TI). The simulation program estimated that light pollution, which disturbs sleep, could beeliminated in the European streetlight case. Determining methods for the light distribution control, performance, and optimal lighting setup conditions is very important to prevent light pollution. Moreover, the initial step of developing the lighting system design and post management will require an effort with much analysis.

MONTE-CARLO RADIATIVE TRANSFER MODEL OF THE DIFFUSE GALACTIC LIGHT

  • Seon, Kwang-Il
    • 천문학회지
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    • 제48권1호
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    • pp.57-66
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    • 2015
  • Monte-Carlo radiative models of the diffuse Galactic light (DGL) in our Galaxy are calculated using the dust radiative transfer code MoCafe, which is three-dimensional and takes full account of multiple scattering. The code is recently updated to use a fast voxel traversal algorithm, which has dramatically increased the computing speed. The radiative transfer models are calculated with the generally accepted dust scale-height of 0.1 kpc. The stellar scale-heights are assumed to be 0.1 or 0.35 kpc, appropriate for far-ultraviolet (FUV) and optical wavelengths, respectively. The face-on optical depth, measured perpendicular to the Galactic plane, is also varied from 0.2 to 0.6, suitable to the optical to FUV wavelengths, respectively. We find that the DGL at high Galactic latitudes is mostly due to backward or large-angle scattering of starlight originating from the local stars within a radial distance of r < 0.5 kpc from the Earth. On the other hand, the DGL measured in the Galactic plane is mostly due to stars at a distance range that corresponds to an optical depth of $${\sim_\sim}$$ 1 measured from the Earth. Therefore, the low-latitude DGL at the FUV wavelength band would be mostly caused by the stars located at a distance of $r{\leq}0.5$ kpc and the optical DGL near the Galactic plane mainly originates from stars within a distance range of $1{\leq}r{\leq}2kpc$. We also calculate the radiative transfer models in a clumpy two-phase medium. The clumpy two-phase models provide lower intensities at high Galactic latitudes compared to the uniform density models, because of the lower effective optical depth in clumpy media. However, no significant difference in the intensity at the Galactic plane is found.