• 제목/요약/키워드: Scattered Light

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Dust Scattering in Turbulent Media: Correlation between the Scattered Light and Dust Column Density

  • Seon, Kwang-Il;Witt, Adolf N.
    • 천문학회보
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    • 제39권1호
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    • pp.59.2-59.2
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    • 2014
  • Radiative transfer models in a spherical, turbulent interstellar medium (ISM), in which the photon source is situated at the center, are calculated to investigate the correlation between the scattered light and the dust column density. The medium is modeled using fractional Brownian motion structures that are appropriate for turbulent ISM. The correlation plot between the scattered light and optical depth shows substantial scatter and deviation from simple proportionality. It was also found that the overall density contrast is smoothed out in scattered light. In other words, there is an enhancement of the dust-scattered flux in low-density regions, while the scattered flux is suppressed in high-density regions. The correlation becomes less significant as the scattering becomes closer to being isotropic and the medium becomes more turbulent. Therefore, the scattered light observed in near-infrared wavelengths would show much weaker correlation than the observations in optical and ultraviolet wavelengths. We also find that the correlation plot between scattered lights at two different wavelengths shows a tighter correlation than that of the scattered light versus the optical depth.

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분할화상분석에 의한 흐름 형태 시료의 탁도 측정 (The Turbidity Measured by Division Image Analysis in Flow Type Sample)

  • 박종호;박수행;유민수
    • 공업화학
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    • 제20권6호
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    • pp.681-684
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    • 2009
  • 흐름 형태 시료의 탁도와 레이저 산란광 밝기의 관계는 비선형적이나 탁도 시료에 따라 레이저 산란광 화상은 형태가 서로 상이하다. 레이저 산란광 화상의 패턴을 이용하면 탁도 측정이 용이할 것이다. 그러나 레이저 산란광 화상의 모든 화소의 red, green, blue intensity (intensity)로 탁도를 측정하는 것은 분석에 과도한 부하가 발생한다. 따라서 과도한 부하를 줄이기 위하여 레이저 산란광 화상 분할하였다. 분할된 레이저 산란광 화상은 탁도에 따라 형태가 서로 상이함을 알 수 있었다. 분할된 레이저 산란광 화상의 intensity와 탁도로 학습된 인공신경망으로 측정된 탁도가 실제 탁도와 선형 관계임을 알 수 있었다.

표면 거칠기 광산란 패턴의 컴퓨터 수치 분석 (I) (Mumerical Anlysis of light Scattering Patterns for Measurement of Roughmess(I))

  • 임동열;김승우
    • 대한기계학회논문집
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    • 제16권2호
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    • pp.267-280
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    • 1992
  • This paper describes a numerical analysis of the light scattering patterns of roughness profiles. This analysis was based upon the light scattering theory developed by Beckmann. In the analysis, the roughness profile was regarded as a profile whose irregularities depend on the production process and the shape of cutting tool. Generally, waviness of an actual surface seriously distorts the scattered pattern of roughness profile. In order to avoid the effects of waviness of actual surfaces, several theoretically calculated scattering patterns, instead of actual scattering patterns, were used to analyze the scattering patterns of typical engineering roughness profiles. The characteristics of the light scattering patterns for five model surfaces were studied.

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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혼탁매질에서 광분포에 관한 Monte Carlo 시뮬레이션 (Monte Carlo Simulation on Light Distribution in Turbid Material)

  • 김기준;성기천
    • 한국응용과학기술학회지
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    • 제15권4호
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    • pp.11-20
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    • 1998
  • The propagation of light radiation in a turbid medium is an important problem that confronts dosimetry of therapeutic laser delivery and the development of diagnostic spectroscopy. Scattered light is measured as a function of the position(distance r, depth z) between the axis of the incident beam and the detection spot. Turbid sample yields a very forward-directed scattering pattern at short range of position from source to detector, whereas the thicker samples greatly attenuated the on-axis intensity at long range of position. The portions of scattered light reflected from or transmitted throughphantom depend upon internal reflectance and absorption properties of the phantom. Monte Carlo simulation method for modelling light transport in tissue is applied. It uses the photon is moved a distance where it may be scattered, absorbed, propagated, internally reflected, or transmitted out of tissue. The photon is repeatedly moved until it either escape from or is absorbed by the phantom. In order to obtain an optimum therapeutic ratio in phantom material, optimum control the light energy fluence rate is essential. This study is to discuss the physical mechanisms determining the actual light dose in phantom. Permitting a qualitative understanding of the measurements. It may also aid in designing the best model for laser medicine and application of medical engineering.

Dust scattering simulation of far-ultraviolet light in the Milky Way

  • Jo, Young-Soo;Seon, Kwang-Il;Witt, Adolf N.;Min, Kyoung-Wook
    • 천문학회보
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    • 제44권2호
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    • pp.48.2-48.2
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    • 2019
  • Light from universe is absorbed, scattered, and re-released by interstellar dust before it reaches us. Therefore, accurate correction of the observed light requires not only spatial distribution of interstellar dust, but also information on absorption and scattering for each wavelength. Far-ultraviolet (FUV) light is mainly produced by bright, young O-type and some B-type stars, but it is also observed in interstellar space without these stars. Called FUV Galactic light (DGL), these lights are mostly known as starlight scattered by interstellar dust. With the recent release of GAIA DR2, not only accurate distance information of stars in our Galaxy, but also accurate three-dimensional distribution maps of interstellar dust of our Galaxy were produced. Based on this, we performed 3-dimensional Monte Carlo dust scattering radiative transfer simulations for FUV light to obtain dust scattered FUV images and compared them with the observed FUV image obtained by FIMS and GALEX. From this, we find the scattering properties of interstellar dust in our Galaxy and suggest the intensity of extragalactic background light. These results are expected to aid in the study of chemical composition, size distribution, shape, and alignment of interstellar dust in our Galaxy.

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광도파관 외부산란광을 이용한 우적감지 센서 (Rain Sensor using Scattered Light Outside Waveguide)

  • 최규남
    • 전자공학회논문지SC
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    • 제48권2호
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    • pp.22-27
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    • 2011
  • 차량의 윈드실드 유리 외면에서의 빗방울에 의한 산란광을 수신하여 빗방울 존재 유무를 판별하는 우적감지 센서를 제안한다. 기존의 윈드실드 유리를 광도파관으로 이용하는 우적감지 센서는 신호광을 윈드실드 유리 내부로 주입하기 위하여 정밀한 광학계를 필요로 하며 외부 진동이나 충격에 의해 광결합률에 영향을 주어 오작동되는 경우가 있었다. 제안하는 광도파관 외부에 존재하는 빗방울에 의한 산란광을 이용하는 우적감지 센서는 광도파관 내부에 신호광을 주입할 필요가 없으므로 별도의 광학계가 필요 없으며 외부 충격이나 진동의 영향을 받지 않는 장점이 있다. 스프레이어를 이용한 가상강우 환경에서, 제작된 광도파관 외부 산란광을 이용한 우적감지 센서에 대한 실험결과는 빗방울뿐만 아니라 안개와 같은 미세한 입자에도 반응하여 차량용 우적감지 센서로 이용할 수 있는 가능성을 보여주었다.

2개의 레이저 파장에 따른 마우스 호중구의 산란광 비교 연구 (Comparison of Scattered Light of ex vivo Mouse Neutrophils by Different Wavelength Laser Irradiation)

  • 박재성;손민지;황창순;이호
    • 한국산업융합학회 논문집
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    • 제25권3호
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    • pp.365-378
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    • 2022
  • Complete blood cell count(CBC) is a technique that counts leukocytes for each type of blood cell being analyzed. The principle is that laser is incident to ex vivo flowing leukocytes in a microcapillary tube and scattered light occurs by laser and leukocytes. By collecting the scattered light, we can count the types of cells because different cells generate different light-scattering patterns. However, the technique has an intrinsic limitation, scattering pattern is shown in a wide range region in the resulting, which makes it difficult to accurate analyze and use fluorescent dyes. To overcome this limitation, a new design of CBC with a dual laser, which irradiates with orthogonal angles for collecting quad-scattering information was proposed. Before development, the scattering difference depending on wavelength must be investigated to only catch up to the scattered signal by angles. Some studies, which focused on simple particles, have been conducted to theoretically and experimentally investigate different scatterings by wavelength. In this study, we propose an optical system for measuring scattered light and investigate a complex particle. As a result, the green laser made strong scattering signals in both the forward and side direction: 10% and 30%, respectively.

실리콘 웨이퍼 미세 표면결함의 광산란 특성 평가 (Light Scattering Characteristics of Defects on Silicon Wafer Surface)

  • 하태호;송준엽
    • 한국정밀공학회:학술대회논문집
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    • 한국정밀공학회 2005년도 춘계학술대회 논문집
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    • pp.1083-1086
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    • 2005
  • Light scattering measurement system that can evaluate light scattering characteristic from defects on silicon wafer surface has been developed. The system uses $Ar^+$ laser as an illumination source, and a highly sensitive photomultiplier tube (PMT) for detecting scattered light from defects. Unlike with conventional measurement system, our system has ability to measure scattered light pattern from wide range of scattering angles with changeable incidence condition. It is shown that our developed system is effective to discriminate the types and sizes of defects from basic experimental results using a microscatch and a PSL sphere.

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Polarization State of Scattered Light in Apertureless Reflection-mode Scanning Near-Field Optical Microscopy

  • Cai, Yongfu;Aoyagi, Mitsuharu;Emoto, Akira;Shioda, Tatsutoshi;Ishibashi, Takayuki
    • Journal of Magnetics
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    • 제18권3호
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    • pp.317-320
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    • 2013
  • We studied the polarization state in an apertureless scanning near-field microscopy (a-SNOM) operating in reflection mode by using three-dimensional Finite-difference Time-domain (FDTD) method. As a result, the electric field around tip apex in the near-field region enhanced four times stronger than the incident light for ppolarization when the tip-sample separation was 10 nm. We find that the p- and s-polarization state is maintained for the scattered light when the probe is perpendicular to the sample. When the probe is not perpendicular to the sample, the polarization state of scattered light will rotate an angle that equals to the inclination angle of probe with p-polarization illumination. On the other hand, the polarization state will not rotate with s-polarization illumination.