• Current Optics and Photonics
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• 제7권4호
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• pp.449-456
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• 2023

The localized surface-plasmon resonance has drawn great attention, due to its unique optical properties. In this work a general theoretical description of the dipole mode is proposed, using the forced damped harmonic oscillator model of free charges in an ellipsoid. The restoring force and driving force are derived in the quasistatic approximation under general conditions. In this model, metal is regarded as composed of free charges and bound charges. The bound charges form the dielectric background which has a dielectric function. Those free charges undergo a collective motion in the dielectric background under the driving force. The response of free charges will not be included in the dielectric function like the Drude model. The extinction and scattering cross sections as well as the damping coefficient from our model are verified to be consistent with those based on the Drude model. We introduce size effects and modify the restoring and driving forces by adding the dynamic depolarization factor and the radiation damping term to the depolarization factor. This model provides an intuitive physical picture as well as a simple theoretical description of the dipole mode of the localized surface-plasmon resonance based on free-charge collective motion.

• 천문학회보
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• 제37권1호
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• pp.73.1-73.1
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• 2012

We present the results of dust scattering simulations carried out for the Orion Eridanus Superbubble region by comparing them with observations made in the far-ultraviolet. The albedo and the phase function asymmetry factor (g-factor) of interstellar grains were estimated as well as the distance and thickness of the dust layers. The results are: 0.39-0.45 for the albedo and 0.25-0.65 for the g-factor, in good agreement with previous determinations and theoretical predictions. The distance of the assumed single dust layer, modeled for the Orion Molecular Cloud Complex, was estimated to be -110 pc and the thickness ranged from -130 at the core to -50 pc at the boundary for the region of the present interest, implying that the dust cloud is located in front of the Superbubble. The simulation result also indicates that a thin (-10 pc) dust shell surrounds the inner X-ray cavities of hot gas at a distance of -70-90 pc.

• 천문학회보
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• 제37권2호
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• pp.98.1-98.1
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• 2012

We present the results of dust scattering simulations carried out for the Orion-Eridanus Superbubble region by comparing them with observations made in the far-ultraviolet. The albedo and the phase function asymmetry factor (g-factor) of interstellar grains were estimated, as were the distance and thickness of the dust layers. The results are as follows: [0.43]_(-0.04)^(+0.02) for the albedo and [0.43]_(-0.2)^(+0.2) for the g-factor, in good agreement with previous determinations and theoretical predictions. The distance of the assumed single dust layer, modeled for the Orion Molecular Cloud Complex, was estimated to be ~110 pc, and the thickness ranged from ~130 at the core to ~50 pc at the boundary for the region of present interest, implying that the dust cloud is located in front of the superbubble. The simulation result also indicates that a thin (~10 pc) dust shell surrounds the inner X-ray cavities of hot gas at a distance of ~70-90 pc.

• 한국자기공명학회논문지
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• 제25권4호
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• pp.51-57
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• 2021

We study optical quantum transition line widths in relation to magnetic field dependence properties of the electrons confined in an infinite square well potential system between z = 0 and z = L_z in the z - direction. We consider two systems-one is subject to right circularly oscillating external fields and the other is subject to left circularly oscillatory external fields. Our results indicate that the line widths of right circularly oscillating external fields is larger than the line widths of left, while the opposite result is obtained for the line widths.

• Nuclear Engineering and Technology
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• 제52권3호
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• pp.461-468
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• 2020

The improvements of the DeCART/MUSAD code system for uncertainty analysis of HTGR neutronic parameters are presented in this paper. The function for quantifying an uncertainty of critical-spectrumweighted few group cross section was implemented using the generalized adjoint B₁ equation solver. Though the changes between the infinite and critical spectra cause a considerable difference in the contribution by the graphite scattering cross section, it does not significantly affect the total uncertainty. To reduce the number of iterations of the generalized adjoint transport equation solver, the generalized adjoint B₁ solution was used as the initial value for it and the number of iterations decreased to 50%. To reflect the implicit uncertainty, the correction factor was derived with the resonance integral. Moreover, an additional correction factor for the double heterogeneity was derived with the effective cross section of the DH region and it reduces the difference from the complete uncertainty. The code system was examined with the MHTGR-350 Ex.II-2 3D core benchmark. The k_eff uncertainty for Ex.II-2a with only the fresh fuel block was similar to that of the block and the uncertainty for Ex.II-2b with the fresh fuel and the burnt fuel blocks was smaller than that of the fresh fuel block.

• Electronic Materials Letters
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• 제14권6호
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• pp.725-732
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• 2018

The thermoelectric and transport properties of Ti-doped FeVSb half-Heusler alloys were studied in this study. $FeV_{1-x}Ti_xSb$ (0.1 < x < 0.5) half-Heusler alloys were synthesized by mechanical alloying process and subsequent vacuum hot pressing. After vacuum hot pressing, a near singe phase with a small fraction of second phase was obtained in this experiment. Investigation of microstructure revealed that both grain and particle sizes were decreased on doping which would influence on thermal conductivity. No foreign elements pick up from the vial was seen during milling process. Thermoelectric properties were investigated as a function of temperature and doping level. The absolute value of Seebeck coefficient showed transition from negative to positive with increasing doping concentrations ($x{\geq}0.3$). Electrical conductivity, Seebeck coefficient and power factor increased with the increasing amount of Ti contents. The lattice thermal conductivity decreased considerably, possibly due to the mass disorder and grain boundary scattering. All of these turned out to increase in power factor significantly. As a result, the thermoelectric figure of merit increased comprehensively with Ti doping for this experiment, resulting in maximum thermoelectric figure of merit for $FeV_{0.7}Ti_{0.3}Sb$ at 658 K.

• 대한원격탐사학회지
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• 제36권2_1호
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• pp.155-165
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• 2020

본 연구에서는 복사전달모델을 사용하여 다양한 변수환경(파장 (340 nm, 477 nm), 에어로솔 종류(스모크, 황사, 황산염), AOD (aerosol optical depth), 지표면 반사도, 관측기하)에 따라 에어로솔 유효 고도(aerosol peak height; APH)에 대한 O₄ 대기질량인자(air mass factor; AMF)의 민감도를 조사하였다. 전반적으로, 477 nm의 O₄ AMF 가 340 nm 보다 APH에 대한 민감도가 크고 안정적으로 산출 가능한 것으로 확인하였다. AOD가 높을 때 APH에 대한 O₄ AMF의 민감도가 커지는 것을 확인하였다. 477 nm에서는 340 nm 보다 지표면 반사도의 영향이 큰 것으로 나타났다. 태양천정각 증가에 따라 340 nm에서의 O₄ AMF가 감소하는 추세를 발견하였으며, 이러한 경향은 태양천정각 40°인 환경에서 높은 Rayleigh 및 Mie 산란에 의한 장벽효과로 인해 O₄ 흡수가 발생하는 광경로 길이가 줄어들기 때문인 것으로 사료된다. 477 nm에서는 태양천정각이 증가함에 따라 Rayleigh 및 Mie 산란에 의한 다중산란이 일부 발생하여 O₄ AMF가 비선형함수 형태로 증가하는 경향을 보였다. 마지막으로, AOD의 불확실성이 APH 산출오차에 미치는 영향을 조사하였다. 황산염 타입에 대한 APH 산출 시, AOD의 불확실성으로 인한APH 산출오차가 다른 에어로솔 타입보다 크게 나타났으며, 황사의 경우 AOD 불확실성에 대한 APH 산출오차에 대한 영향이 미미하게 나타났다. 이러한 결과는 각 에어로솔 타입의 흡수 산란 특성이 다양하기 때문에, 에어로솔 타입이 APH 산출 오차에 영향을 미칠 수 있음을 의미한다.

• 한국가시화정보학회지
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• 제12권3호
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• pp.9-14
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• 2014

Two-photon microscopy (TPM) has been used in plant research as a high-resolution high-depth 3D imaging modality. However, TPM is known to induce photo-damage to the plant in case of long time exposure, and optimal excitation wavelength for plant imaging has not been investigated. Longer excitation wavelength may be appropriate for in vivo two-photon imaging of Arabidopsis thaliana leaves, and effects of longer excitation wavelength were investigated in terms of imaging depth, emission spectrum. Changes of emission spectrum as a function of exposure time at longer excitation wavelength were measured for in vivo longitudinal imaging. Imaging depth was not changed much probably because photon scattering at the cell wall was a limiting factor. Chloroplast emission spectrum showed its intensity peak shift by 20 nm with transition of excitation wavelength from 849 nm or below to 850 nm or higher. Emission spectrum showed different change patterns with excitation wavelengths in longitudinal imaging. Longer excitation wavelengths appeared to interact with chloroplasts differently in comparison with 780 nm excitation wavelength, and may be good for in vivo imaging.

• 한국음향학회지
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• 제31권3호
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• pp.115-128
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• 2012

본 연구는 확산체의 확산계수 측정결과를 바탕으로 확산체의 설치가 홀 내부 음장분포에 미치는 영향에 대하여 알아보았다. 오케스트라쉘이 설치된 600석 규모의 축소모형 홀을 측정대상으로 이용하였다. 잔향실법 흡음률 측정을 통해 1: 25 축소모형의 벽체와 객석부 재료 (관객 및 의자)가 선정되었고, 만석 시 잔향시간을 기준으로 컴퓨터 시뮬레이션과 대응되도록 제작하였다. 다양한 확산체 부착위치에 따른 물리적 음장의 변화를 측정하기 위해 반구 확산체를 측벽, 발코니전면, 천장 등 부위별로 7가지 조합을 만들어, 확산체 유/무에 따른 음향지표의 변화를 측정하였다. 사용된 음향지표는 잔향시간 (RT), 초기감쇠시간 (EDT), 명료도 (C80), 중심시간 (Ts), 음압레벨 (G)과 더불어 임펄스리스펀스의 자기상관함수 (ACF)로부터 도출되는 Temporal diffusion (TD)을 이용하였다. 실험결과, 확산체 설치에 따라 흠음력과 확산면적이 증가하였고, 이에 따라 평균 RT, 평균 EDT, 평균 G는 감소하는 경향을 보였다. 또한 확산체 설치로 인해 초기반사음의 방향전환이 활발하게 발생했고, 평균 TD은 측정 케이스에 따라 6.05에서 6.30의 값을 보였다. 확산체 설치에 가장 민감한 지표는 RT (R = 0.94)로 나타났고, TD와 EDT의 상관관계 (R = 0.73)가 높은 것으로 나타났다. 확산체 설치부위의 영향은 각 음향지표의 변화양상을 통해 논의되었다.

• 대한원격탐사학회지
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• 제30권1호
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• pp.47-59
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• 2014

화산재입자의 굴절률과 산란 같은 고유 광학 특성으로 결정되는 분광학적 신호는 원격탐사 센서를 통하여 측정될 수 있지만, 화산 폭발 이후 생성된 화산재입자의 성분에 대한 굴절률에 관한 정보는 매우 제한적이었다. 따라서, 화산재입자의 원격탐사의 강건성을 개선하기 위하여 화산재입자와 복사전달 과정의 상호작용에 대한 정확한 이해가 필요하다. 본 연구에서는 화산재 주요 성분으로 알려진 화산성 안산암과 부석에 대한 입자 소산계수, 산란 위상함수, 비대칭 계수, 단산란 알베도 값을 정량화 하였다. 이러한 화산재입자의 고유 광학 특성값은 복사전달모델의 입력자료로 이용하여 다양한 에어러솔 광학두께(${\tau}$) 및 기하조건에서 원격탐사 센서(인공위성과 지상관측용)가 측정하는 이론적인 복사량과 화산재입자 특성의 관계를 분석하였다. 복사전달모델 분석결과, 대기권 최상층부에서 ${\tau}$ 에 대한 복사량의 변화율의 평균값은 안산암의 경우 부석보다 6배 정도 크게 나타났다. 지표에서 이러한 변화율은 ${\tau}$ <1인 경우 양의 상관관계를 보이지만, ${\tau}$ >1인 경우에는 음의 상관관계를 보였다. 그러나, 적외선 영역인 11 ${\mu}m$ 에서는 차이가 매우 적게 나타났으며, 여기서 발생하는 복사량의 오차범위는 광학두께가 증가할수록 커지는 양상을 보이며, 다항 회귀함수로 표현될 수 있다. 이러한 결과는 원격 탐사 관측자료를 이용한 화산재 관측에 있어서 화산재의 정량적 분석에 도움이 될 것이다.