• Title/Summary/Keyword: light flux ratio

검색결과 39건 처리시간 0.025초

Illuminance Distribution and Photosynthetic Photon Flux Density Characteristics of LED Lighting with Periodic Lattice Arrangements

  • Jeon, Hee-Jae;Ju, Kang-Sig;Joo, Jai-Hwang;Kim, Hyun-Gyun
    • Transactions on Electrical and Electronic Materials
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    • 제13권1호
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    • pp.16-18
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    • 2012
  • LED lighting systems that combine lighting capability, emotional and physiological characteristics are required for lighting source and multifunctional applications. In this work, Simulation studies using optical analysis software packages, Light Tools, are presented. This is done to estimate the uniformity ratio of illuminance and photosynthetic photon flux density (PPFD) of the periodic 2D lattice arrangements, such as square, diamond, two-way bias quadrangular, hexagonal, and Kagome lattices, under the same transmissivity, absorptance and reflectivity. It has been found out that the two-dimensional Kagome lattice arrangement exhibited high uniformity ratio of illuminance and PPFD compared to other lattices. Accordingly, these results can be used to guide a design and improve the lighting environment which in turn would maximize the uniform distributions of illuminance.

기상 측정을 위한 광학적 표면 거칠기 측정 센서 개발 (Development of An Optical Surface Roughness Sensor for On-the-Machine Measurement)

  • 김현수;홍성욱
    • 한국정밀공학회지
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    • 제11권6호
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    • pp.168-178
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    • 1994
  • This paper presents an optical surface roughness sensor developed for intermediate- process measurement on the machine. The light scattering method is adopted for the sensor, which is designed conpact and flexible enough to apply to 'on the machine' measurement of surface roughness. The developed sensor has special features such that it makes use, as the measurement parameter, of the ratio between fluxes of the incident light, and the specularly and partly diffusely reflected light, and that it can adjust the incident light angle. The experimental investigation reveals not only the sensor has good performance as a surface roughness sensor but the sensor is very robust so as to be useful in in-process measurement.

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Monitoring observation of PG0934+013 using The Southern African Large Telescope

  • Park, Dawoo;Woo, Jong-Hak;Romero-Colmenero, Encarni;Crawford, Steven M.;Barth, Aaron J.;Pei, Liuyi
    • 천문학회보
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    • 제38권2호
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    • pp.54-54
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    • 2013
  • We performed spectroscopic and photometric monitoring observations of a QSO, PG0934+013 for a reverberation-mapping analysis, using the 9-m Southern African Large Telescope (SALT) for spectroscopy and the 2-m Faulkes Telescope North and the South for photometry. The monitoring campaign was carried out for 5 month between December 2012 to April 2013, providing 20 spectroscopic epochs and ~40 photometric epochs. Based on the obtained spectra, which typically have a signal-to-noise ratio to 30-60, we performed multicomponent decomposition using various components, i.e., power-law continuum, FeII emission complex, and broad and narrow emission lines, to properly measure the Hbeta line flux. After a flux normalization using [O III] 5007 line luminosity, we obtained a rms spectrum from all epochs, which shows clear variability of Hbeta line. We find that Hbeta line flux decreases by ~20% during the monitoring period while the continuum flux obtained from the aperture photometry based on the imaging data, shows similar variability. The current Hbeta light curve shows monotonic decrease and a reliable cross correlation analysis between Hbeta and continuum light is difficult. Nevertheless, we obtained a preliminary lag measurements as ~24 light days.

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식물생장용 고압나트륨램프와 메탈할라이드램프의 분광 광강도 분석 (Analysis of Spectral Light Intensity of High Pressure Sodium and Metal Halide Lamps for Plant Growth)

  • 이혜인;김용현;김동억
    • Journal of Biosystems Engineering
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    • 제35권6호
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    • pp.413-419
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    • 2010
  • Plant growth was greatly affected by the spectral distribution and light intensity of artificial lighting sources. In this study, the spectral characteristics of high power sodium (HPS) lamps and metal halide (MH) lamps produced by three different manufacturers were measured. Even though the spectral distribution of HPS lamps with lamp wattage of 250 W and 400 W was very similar, but the spectral light intensity by the manufacturers was different. Difference in the spectral light intensity of MH lamps by the manufacturers was increased with the increasing lamps wattage. Light intensity at the region of blue (B), green (G), red (R) and far-red (FR) light of HPS and MH lamps was also analyzed. HPS lamps showed the light intensity in order of R, FR, B and G light. The ratio of G, B, R and FR to photosynthetic photon flux (PPF) of HPS lamps with the lamp wattage of 250 W was 3.0-3.2%, 5.5-5.9%, 17.3-19.2% and 6.5-7.8%, respectively. For MH lamps, it showed the light intensity in order of R, FR, B, and G. The ratio of B, G, R, and FR to PPF of MH lamps with 250 W was 14.0-15.5%, 22.6-27.5%, 7.5-9.5% and 2.7-4.2%, respectively. HPS and MH lamps with 400 W had a relatively smaller ratio of R and FR to PPF than those with 250 W. HPS lamps showed that the ratio of light intensity of B and FR to R was 0.15-0.28 and 0.36-0.4, respectively. For MH lamps, the ratio of light intensity of B and FR to R was 1.26-2.72 and 0.27-0.56, respectively. From these results, it was concluded that the portion of blue light of MH lamps was higher than those of HPS lamps.

연삭기에서의 기상 측정 (On-machine Measurement for grinding Machines)

  • 김현수;홍성욱
    • 한국정밀공학회지
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    • 제18권6호
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    • pp.27-36
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    • 2001
  • 본고에서는 고정도 제품을 생산하는 연삭기에 대해 가공물 및 연삭 공구인 연삭 숫돌을 기상에서 측정하기 위한 여러 가지 방법들을 소개하였고 일부는 적응 예를 기술하였다. 소개된 기상 측정장치들은 특히 반복 공정이 필요한 연삭 현장에서 생산성 향상을 위해 유용하게 활용될 수 있을 것으로 생각된다. 그러나 관련 연구가 지속된다면 연삭기의 작업조건 자동 설정, 연삭 상태 진단 등, 연삭기의 지능화에도 적극적으로 응용될 수 있을 것으로 기대된다.

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산란광속측정에 의한 연삭가공 표면 거칠기 측정방법 (A Method for Measurement of Roughness of Ground Surfaces by Using Fluxes of Scattered Lights)

  • 홍성욱;김현수
    • 한국정밀공학회지
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    • 제12권4호
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    • pp.46-54
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    • 1995
  • This paper presents a simple method for measurenemt of roughness of ground surfaces. The present method utilizes fluxes of scattered lights condensed through lenses aligned along the specular direction. A theoretical analysis is preformed for the purpose of investigating the possibility of the method as well as determining the experimental condition. Experiments are also performed to show the effectiveness and robustness of the proposed method. The theoretical and experimental results show that the proposed method is simple enouth to implement and has a potential to identify a wide range of roughness of ground surfaces.

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Growth and Flowering Responses of Petunia to Various Artificial Light Sources with Different Light Qualities

  • Park, In Sook;Cho, Kyung Jin;Kim, Jiseon;Cho, Ji Yoon;Lim, Tae Jo;Oh, Wook
    • 원예과학기술지
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    • 제34권1호
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    • pp.55-66
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    • 2016
  • This study was carried out to investigate the effect of artificial light sources with different light qualities on the growth and flowering characteristics of a herbaceous long-day plant, Petunia ${\times}$ hybrida Hort. Seedlings of petunia cultivar 'Madness Rose' were potted, acclimated for one week, and grown in a phytotron equipped with tube- and bulb-type fluorescent lamps (FL tube and bulb), tube-type white light-emitting diodes (LED tube), halogen lamps (HL), metal halide lamps (MH), and high pressure sodium lamps (HPS) for 10 weeks. The temperature, photoperiod, and photosynthetic photon flux density (PPFD) in the phytotron were $22{\pm}2^{\circ}C$, 16 h, and $25{\pm}2{\mu}mol{\cdot}m^{-2}{\cdot}s^{-1}$, respectively. Light sources combined with HL promoted stem elongation, and plant height and internode length decreased with increasing red to far-red (R:FR) ratio. FL tube + LED tube, HPS, and FL tube promoted branching, whereas plants grown under light sources combined with HL did not have any branches. Days to flowering (from longest to shortest) occurred as follows: FL tube + HL > FL tube + HL > MH > HPS = FL tube + FL bulb > FL tube + LED tube > LED tube > FL tube, indicating that reducing the R:FR ratio of the light sources promoted flowering. Only 20% of plants grown under an FL tube flowered, whereas under all other treatments, 100% of plants flowered. At 10 weeks after treatment, plants grown under HPS and MH had (cumulatively) 12 open flowers, and those grown under FL tube + FL bulb, LED tube, FL tube + LED tube, and HPS treatment had approximately seven flower buds. These results suggest that light sources with low R:FR ratios promote flowering and stem elongation in petunia, but they reduce its ornamental value due to overgrowth and poor branching.

Multiple Light Scattering 분석법을 이용한 천연수경성석회의 초기경화 거동 (Early Hardening Behavior of Natural Hydraulic Lime Paste by Multiple Light Scattering Analysis)

  • 문기연;조계홍;조진상;홍창우
    • 자원리싸이클링
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    • 제26권1호
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    • pp.43-50
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    • 2017
  • 본 연구에서는 무기질 첨가재를 혼합한 천연수경성석회의 초기경화 거동분석을 위해 multiple light scattering 분석법을 이용하였다. 자체 제조한 천연수경성석회의 물성향상을 위해 고로수쇄슬래그 및 3종류의 석고를 혼합비에 따라 혼합하였으며 물-고체비 0.6으로 페이스트를 제조하였다. 제조한 페이스트를 이용하여 원통형의 용기에 일정량을 담아 장비(Turbiscan LAB, Formulaction)에 장입하여 분석을 실시하였다. 페이스트로부터의 backscattering flux(BS, %)는 $23^{\circ}C$의 온도에서 분석용기 전체높이(55 mm)에 대해 24시간 동안 10분 간격으로 측정되었다. 모든 시료에서 전체적으로 BS는 시간경과에 따라서 증가하는 경향성을 보였다. 고로수쇄슬래그와 석고를 첨가함에 따라서 시간에 따른 BS의 증가 속도는 0.02에서 0.38 BS %/hour 까지 증가하였다. 반수석고를 혼합하였을 경우 가장 높은 backscattering flux와 BS의 증가속도를 보였다.

발광영상에 대한 정량화 방법 개발 (Development of Quantification Method for Bioluminescence Imaging)

  • 김현식;최은서;탁윤오;최흥국;이주영;민정준;이병일
    • Nuclear Medicine and Molecular Imaging
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    • 제43권5호
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    • pp.451-458
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    • 2009
  • 목적: 광학적 분자 발광영상은 발광효소를 이용하여 발광하는 빛의 신호를 영상화하는 기법이다. 발광하는 광량이 분자 변화 또는 세포 수와 비례하고 신호 대 잡음비가 좋아서 영상을 얻고, 정략분석이 가능하다. 이 연구에서는 정량적 분석을 위해 비례적 측정 정량화기법을 개발하였다. 대상 및 방법: 개발 중인 ALIS (animal light imaging system) 광학발광영상 카메라에서 박테리아 수를 달리한 박테리아 광원 3가지와 또 다른 3가지 광원을 이용하여 발광영상을 측정하였다. 일정한 세기의 광원에 대해서 측정 방법을 수학적으로 표현하기 위해 cd와 광속의 개념을 이용하여 간단한 수식을 유도하였다. 실험을 통해 측정시간 1초를 기준으로 얻어진 값으로 표준 정량화 함수를 얻었다. 얻어진 정량화 함수를 이용하여 박테리아를 이용한 실험에 필요한 함수의 상수 값을 구했으며, 세 가지 세기가 다른 광원을 이용하여 측정한 값을 측정시간과 함께 정량화 식에 대입하여 측정하였다. 결과: 표준측정함수를 이용하여 측정시간에 비례하는 정량적 값을 얻을 수 있었다. 정량화결과를 측정시간으로 나눠준 값은 일정하였으며, 측정시간에 대비한 비례적 값을 얻을 수 있었다. 결론: 측정한 결과를 정량화 함수에 대입하여 정량화시킨 값은 표준정량화 하기에 적합하였다. 이 정량화 방법은 다른 광학적 분자영상 장비에 적용하여도 빛의 세기를 표준화 시킬 수 있을 뿐 만 아니라 성격이 다른 각각의 광원에 대해서도 보다 정량적인 분석을 시행할 수 있으므로, 새로운 표준 정량화 방법으로 발전시킬 수 있을 것으로 기대한다.

A MONTE CARLO STUDY OF FLUX RATIOS OF RAMAN SCATTERED O VI FEATURES AT 6825 Å AND 7082 Å IN SYMBIOTIC STARS

  • Lee, Young-Min;Chang, Seok-Jun;Heo, Jeong-Eun;Hong, Chae-Lin;Lee, Hee-won
    • 천문학회보
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    • 제41권2호
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    • pp.57.3-58
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    • 2016
  • A symbiotic star is a wide binary system consisting of a hot white dwarf and a mass losing giant, where the giant loses its material in the form of a slow stellar wind resulting in accretion onto the white dwarf through gravitational capture. Symbiotic stars are known to exhibit unique spectral features at 6825 and 7082, which are formed from O VI 1032 and 1038 through Raman scattering with atomic hydrogen. In this Monte Carlo study we investigate the flux ratio of 6825 and 7082 in a neutral region with a geometric shape of a slab, cylinder and sphere. By varying the amount of neutral hydrogen parametrized by the column density along a specified direction, we compute and compare the flux ratio of Raman scattered O VI 6825 and 7082. In the column density around 1020 cm-2, flux ratio changes in a complicated way, rapidly decreasing from the optically thin limit to unity the optically thick limit as the column density increases. It is also notable that when the neutral region is of a slab shape with the O VI source outside the slab, the optically thick limit is less than unity, implying a significant fraction of O VI photons escape through Rayleigh scattering near the boundary. We compare our high resolution CFHT data of HM Sge and AG Dra with the data simulated with finite cylinder models confirming that 'S' type symbiotic tend to be characterized by thicker HI region that 'D' type counterparts. It is expected that this study will be useful in interpretation of the clear disparity of Raman O VI 6825 and 7082 profiles, which will shed much light on the kinematics and the asymmetric distribution of O VI material around the hot white dwarf.

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