• 한국전자파학회논문지
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• 제24권3호
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• pp.324-330
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• 2013

본 논문은 대기압 환경에서 발생하는 유전체 장벽 방전(dielectric barrier discharge: DBD) 플라즈마의 전자파 산란 특성을 측정하였다. 본 논문에서는 기본적인 DBD 플라즈마 발생기 구조를 병렬로 연결하여 넓은 면적의 플라즈마 발생기를 제작하였고, 14 kV, 4 kHz의 고전압 발생장치를 이용해 플라즈마가 발생하는 것을 확인하였다. 두 개의 혼 안테나와 벡터 네트워크 분석기를 이용해 S-parameter의 비교를 통해 전자파 산란 특성을 측정하였다. 전방 산란의 경우 제작된 플라즈마 발생기의 구조적 특성으로 인해 안테나의 편파에 따라 다른 결과 값을 얻었다. 편파가 수평일 때 최대 2 dB의 산란파 감쇠 특성을 확인할 수 있었다. 또한, 편파가 수평일 경우, 플라즈마 발생기 뒤에 PEC를 설치한 후 후방 산란 특성을 측정하였다. 그 결과, 5 GHz에서 안테나 관찰 각도가 $40^{\circ}C$, $60^{\circ}C$일 때 최대 2 dB 산란파 감쇠 특성을 얻었다.

• 한국항공우주학회지
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• 제40권9호
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• pp.737-744
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• 2012

유한체적법을 이용하여 설정된 가상의 노즐 조건에 따라 비행체 배기플룸의 SE와 PE에 의한 열복사 저부가열 해석 연구를 수행하였다. 저부면에서의 복사열유속을 얻기 위해 배기플룸은 흡수, 방사 및 산란하는 매질을 고려하였다. 저부면은 차가운 흑체이고 비회색가스와 입자의 복사 물성치는 회색가스가중합법(WSGGM)을 사용하였다. 후방 몬테카를로 방법을 사용한 기존의 연구와 비교하여 검증한 후, 입자의 농도, 온도, 그리고 등방성 또는 이방성 산란에 따른 복사저부가열을 해석하였다. 그 결과, 복사열유속은 노즐 출구와의 거리가 멀어지거나 비행 고도가 증가할수록 감소하고 입자의 온도가 높아질수록 복사열유속은 증가한다. 또한 전방산란은 PE를 증가시키고 후방산란은 SE를 증가시켰다.

• 대한방사선기술학회지:방사선기술과학
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• 제21권2호
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• pp.43-46
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• 1998

When a patient was irradiated with prosthetic hip, the dose distribution was changed according to inhomogeneous materials. The density, effective atomic number, and the composition of material had influence on absorbed dose distribution. In this study, the influence of inhomogeneous material(Ti) was measured using a polyethylene phantom, which consisted of various diameter of titanium, with film dosimetry. As a result, the backward dose showed 29.5% increas by backscattering, the forward dose showed 28% decreas by absorption, and the side dose showed 7% increas by scattering, when 25 mm diameter Ti was used. In addition forward dose was in inverse proportion to the thickness of prosthetic material. When the prosthetic hip of patient is in an irradiated field, we must carefully study the absorbed dose distribution.

• 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.

• 대한기계학회논문집B
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• 제28권1호
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• pp.59-65
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• 2004

The configuration of intake port and piston is a dominant factor of inlet air flow and mixture formation in an engine cylinder, resepectively. This study has analyzed intake port and piston characteristics for swirl flow of a heavy-duty LPG engine. As an available technology to optimize intake port, the steady flow rig test has been applied for measuring swirl ratio and mean flow coefficient. And we measured the mean velocity and turbulence intensity of swirl flow under motoring condition in transparent engine cylinder by backward scattering LDV system. From these results, the piston and cylinder head with a good evaluated swirl flow characteristics were developed and adapted fur a 11L heavy-duty engine using the liquid phase LPG injection (LPLI) system. The obtained results are expected to be a fundamental data for developing intake port and piston.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2001년도 춘계학술대회 논문집 유기절연재료 전자세라믹 방전플라즈마 연구회
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• pp.201-203
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• 2001

This paper describes the information for quantitative simulation of weakly ionized plasma. We must grasp the meaning of the plasma state condition to utilize engineering application and to understand materials of plasma state. In this paper, the drift velocity of electron in Xenon gas calculated for range of E/N values from 0.01~500[Td] at the temperature is $300[^{\circ}K]$ and pressure is 1[Torr], using a set of electron collision cross sections determined by the authors and the values of drift velocity of electrons are obtained for TOF, PT, SST sampling method of Backward Prolongation by two term approximation Boltzmann equation method. it has also been used to predict swarm parameter using the values of cross section as input. The result of Boltzmann equation, the drift velocity of electrons, has been compared with experimental data by L. S. Frost and A. V. Phelps for a range of E/N. The swarm parameter from the study are expected to server as a critical test of current theories of low energy scattering by atoms and molecules.

• 조명전기설비학회논문지
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• 제29권5호
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• pp.26-33
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• 2015

Secondary optical system designed for LED bulb which emits light in all directions was simulated with Energy Star standards. Components of the optical system were LED light source, the cover of the LED bulb and reflector which is to confirm the diffuser plate and LightTools software was used to design the illumination optics. The main points of the secondary optical system design are the location of the LED light source, the shape of the LED bulb cover, the location of the reflection plate, and the scattering properties of the diffusing plate. Mechanism of the LED bulb is that the light emitted from the light source move on to the backward after reflected by the coated light cover from the inside and then the reflected light is scattered by the diffuser plate. The LED bulb was designed to satisfy the standard light distribution and color specifications of the Energy Star(IES LM-79-08).

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2005년도 하계학술대회 논문집 Vol.6
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• pp.17-18
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• 2005

실리콘 기판 위에 100nm의 선폭을 갖는 선들이 일정한 간격을 가지고 연속적으로 배열되어 있는 구조를 형성시켜 보았다. PMMA가 코팅되어 있는 실리콘 기판위에 전자빔으로 패턴을 하였고, 건식에칭을 통해 구조물을 형성한 후 원자 현미경으로 관찰하였다. 이러한 나노구조물의 구현은 전자빔 패터닝시에 전자빔이 실리콘 기판에 충돌할 때 나타나는 backward scattering과 proximity 효과 등의 영향으로 인해 pitch의 크기가 작아질수록 구현하기가 쉽지 않았다. 화합물반도체 단일 나노선 소자를 제작하여 소자의 전기적 특성을 측정할 때, 나노선 표면에 있는 자연산화막은 금속전극과 나노선 사이의 전기전도특성을 저해하는 요소로 알려져 있다. 이러한 자연산화막을 제거하기 위해 나노선을 건식에칭해 보았고, 원자현미경을 통해 에칭에 따른 나노선의 모양변화를 관찰하였다.

• 한국광학회지
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• 제32권3호
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• pp.120-125
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• 2021

본 연구에서는 다파장 빔결합을 위한 master oscillator power amplifier (MOPA) 구조의 선편광 고출력 이터븀 첨가 광섬유 레이저를 개발하였다. 유도 브릴루앙 산란(stimulated Brillouin scattering, SBS)을 억제하기 위하여 pseudo-random binary sequence (PRBS) 신호로 위상 변조 및 비트길이를 최적화한 선폭 약 10 GHz의 시드 레이저를 구현하였으며, 이를 이용하여 3단 증폭을 하였다. 주 증폭단에서는 모드 불안정성 현상(mode instability, MI)의 문턱값을 높이기 위하여 코어 및 클래딩의 직경이 각각 20 ㎛, 40 ㎛인 편광유지(polarization maintaining, PM) 이터븀 첨가 광섬유를 이용하고 지름이 약 9-12 cm인 나선형 홈에 적용하였다. 그 결과, 입사된 여기광 대비 기울기 효율이 83.7%인 1.004 kW의 레이저 출력을 얻었다. 또한, 빔품질(M²)과 편광소광율(polarization extinction ratio, PER)은 각각 1.12와 21.5 dB로 측정되었다. 더욱이, 역방향 스펙트럼의 레일리 신호와 SBS 신호의 첨두 세기 비율은 2.36 dB로 관측되어, SBS가 완화된 레이저 구현을 확인하였다. 또한 증폭 출력에 따라 기울기 효율 및 빔품질의 저하가 없어 모드불안정이 발생하지 않음을 확인하였다.

• 대기
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• 제18권4호
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• pp.287-297
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• 2008

The vertical profiles and optical properties of Asian dust are investigated using ground-based measurements from 1998 to 2002. Vertical profiles of aerosol extinction coefficient are evaluated using MPL (Micro Pulse Lidar) data. Optical parameters such as aerosol optical thickness ($\tau$), ${\AA}ngstr\ddot{o}m$ exponent ($\alpha$), single scattering albedo ($\omega$), refractive index, and volume size distribution are analyzed with sun/sky radiometer data for the same period. We can separate aerosol vertical profiles into three categories. First category named as 'Asian dust case', which aerosol extinction coefficient is larger than $0.15km^{-1}$ and dust layer exists from surface up to 3-4km. Second category named as 'Elevated aerosol case', which aerosol layer exists between 2 and 6km with 1-2.5km thickness, and extinction coefficient is smaller than $0.15km^{-1}$. Third category named as 'Clear sky case', which aerosol extinction coefficient appears smaller than $0.15km^{-1}$. and shows that diurnal variation of background aerosol in urban area. While optical parameters for first category indicate that $\tau$ and $\alpha$ are $0.63{\pm}0.14$, $0.48{\pm}0.19$, respectively. Also, aerosol volume concentration is increased for range of 1 and $4{\mu}m$, in coarse mode. Optical parameters for second category can be separated into two different types. Optical properties of first type are very close to Asian dust cases. Also, dust reports of source region and backward trajectory analyses assure that these type is much related with Asian dust event. However, optical properties of the other type are similar to those of urban aerosol. For clear sky case, $\tau$ is relatively smaller and $\alpha$ is larger compare with other cases. Each case shows distinct characteristics in aerosol optical parameters.