• 대한기계학회논문집B
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• 제30권10호
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• pp.957-965
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• 2006

A high-performance hot chuck is designed as a heating device for an ultra-precision flip-chip bonder with infrared alignment system. Analysis of design requirements for thermal performance leads to a radiative heating mechanism employing two halogen lamps as heating source. The heating tool is made of silicon carbide characterized by high thermal diffusivity and small thermal expansion coefficient. Experimental tests are performed to assess heat-up performance and temperature uniformity of the heating tool. It is revealed that the initial design of hot chuck results in a good heat-up speed but there exist a couple of troubles associated with control and integrity of the device. As a means to resolve the raised issues, a revised version of heating tool is proposed, which consists of a working plate made of silicon carbide and a supporting structure made of stainless steel. The advantages of this two-body heating tool are discussed and the improved features are verified experimentally.

• 천문학회지
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• 제3권1호
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• pp.1-5
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• 1970

The earlier findings on the radiative heating through the umbral walls in large sunspots are further investigated. No significant evidence for the umbra! heating has been found in small-sized sunspot umbrae.

• 천문학회보
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• 제43권2호
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• pp.52.2-52.2
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• 2018

The shape of a galaxy's spectral energy distribution ranging from ultraviolet (UV) to infrared (IR) wavelengths provides crucial information about the underlying stellar populations, metal contents, and star-formation history. Therefore, analysis of the SED is the main means through which astronomers study distant galaxies. However, interstellar dust absorbs and scatters UV and optical light, re-emitting the absorbed energy in the mid-IR and Far-IR. I present the updated 3D Monte-Carlo radaitive transfer code MoCafe to compute the radiative transfer of stellar, dust emission through a dusty medium. The code calculates the emission expected from dust not only in pure thermal equilibrium state but also in non-thermal equilibrium state. The stochastic heating of very small dust grains and/or PAHs is calculated by solving the transition probability matrix equation between different vibrational, internal energy states. The calculation of stochastic heating is computationally expensive. A pilot study of radiative transfer models of SEDs in clumpy (turbulent), galactic environments, which has been successfully used to understand the Calzetti attenuation curves in Seon & Draine (2016), is also presented.

• 천문학회보
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• 제45권1호
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• pp.70.3-70.3
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• 2020

Previous numerical simulations on planet-disk interactions revealed a lot of interesting phenomena including the planetary migration and the formation of many sub-structures inside the disks. However, these simulations were limited to an isothermal or adiabatic equation of state which does not account for various heating and cooling processes in the disks. Recent studies showed that the behavior of the planet-disk interaction can be significantly influenced by the disk thermodynamics. We develop a radiative diffusion module based on the two-temperature flux-limited diffusion approximation accounting for viscous heating and the accretion feedback. In this presentation, we describe our radiative diffusion solver, present some test results, and discuss potential applications of the module to planet-disk interactions,

• 설비공학논문집
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• 제20권8호
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• pp.563-569
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• 2008

Radiative, heating is suitable for outdoor heating system in windy and cold seasons. Optimal design of the reflector is very important to maximize heat transfer to a specific target area in the open space. The geometrical optical theory can be applied to analyze efficiency of the reflector. Commercial ray tracing computer programs are available only for limited geometries of the reflector. Alternatively, it may be designed and analyzed through an approximated simple lens theory. Two types of reflectors are analyzed using either of these methods. The key issue in this paper is to propose a new illumination experimental method for determination of the radiative efficiency. Optical light source and illuminometer are employed. The calculated efficiency of the reflector is compared with experimental one for checking the reliability. The relative errors between the experimental and analytical results are less than 5%, which proves the validity of this method. Based on these methodologies, a practical reflector and heating lamp unit is developed.

• 한국전산유체공학회지
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• 제12권4호
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• pp.7-13
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• 2007

Numerical analysis is carried out for combined heat transfer in an indirected NIR(Near Infrared Ray) heating chamber. Reynolds number and shapes of absorbed cylinder are known as important parameters on the combined heat transfer effects. Reynolds number based on the outer diameter of the cylinder is varied from $10^3$ to $3{\times}10^5$. Four difference heat transfer regimes are observed: forced convection and radiative heat transfer on the outer surface of the cylinder, pure conduction in the cylinder body, pure natural convection and radiation between lamp surface and inner surface of the cylinder, and radiation from the lamp. Flow and temperature characteristics are presented with iso-contour lines for the absorbed circular and elliptic cylinders to compare their differences. The convective and radiative heat transfer fluxes are also compared with different Reynolds numbers. As usual, Reynolds number is an important factor to estimate increasing convective heat transfer as it increases. The shape of absorbed cylinder results overall heat transfer rates remain unchanged.

• 한국환경과학회:학술대회논문집
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• 한국환경과학회 2003년도 International Symposium on Clean Environment
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• pp.51-54
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• 2003

We analyzed radiative properties of aerosols, $CO^{2}$ and clouds using Optical Properties of Aerosols and Clouds(OPAC) and the Column Radiation Model (CRM). From OPAC, if the soot component is disregarded, dust-like components depict the highest extinction values in the solar spectral range and the lowest. single scattering albedoes, which are attributable to the presence of large particles. In the dust aerosol, the high absorptivity in the infrared may induce a warming of the lower atmospheric layer in the nighttime. The radiative properties of aerosols, clouds and double $CO^{2}$ using the CRM model at Seoul (37N, 127.4 E) on 3 April 2003 were calculated. The solar zenith angle is 65˚ and the surface albedo is 0.1836 during the clear day. The aerosol optical depth change 0.14 to 1.7, which is derived during Asian dust days in Korea. At this time, abedo by aerosols is considered as 0.3. In cloudy condition, the short wave cloud forcing on both the TOA and the surface is -193.89 $Wm^{-2}$ and -195.03 $Wm^{-2}$, respectively, and the long wave cloud forcing is 19.58 $Wm^{-2}$ and 62.08 $Wm^{-2}$, respectively. As a result, the net radiative cloud forcing is -174.31 $Wm^{-2}$ and -132.95 $Wm^{-2}$, respectively. We calculate also radiative heating rates by double $CO^{2}$ during the clear day. The $CO^{2}$ volumn mixing ratio is 3.55E-4.

• 대기
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• 제23권1호
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• pp.85-92
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• 2013

2001년 4월 제주 고산기후관측소에서 AERONET sun/sky radiometer와 MPL을 통해 관측된 에어로졸 광학적 두께, 단산란 알베도, 비대칭 변수, 에어로졸 소산계수 프로파일 등을 대기복사모델의 입력 자료로 이용하여 대기가열효과를 산정하고, 이들 광학변수가 대기복사가열률에 미치는 영향을 분석하였다. 본 연구에서는 NCAR Climate Community Model (CCM-3.6)에 포함되어 있는 복사 모듈인 Column Radiation Model (CRM-2.1.2)을 연직 54층으로, AERONET sun/sky radiometer로부터 관측된 4 파장 (440, 670, 870, 그리고 1020 nm)에서의 관측 자료를 19개의 파장에서 계산 가능하도록 수정하였다. 에어로졸층이 존재하지 않은 맑은 날 (4월 14일과 16일)은 지표면과 대기상단에서의 에어로졸 직접복사강제력이 각각 $-20{\sim}-25\;W\;m^{-2}$와 $-10{\sim}-15\;W\;m^{-2}$로, 대기 중 흡수는 $+10{\sim}+15\;W\;m^{-2}$였다. 에어로졸층이 관측된 4월 15일과 4월 17~18일의 경우 지표면, 대기, 대기상단의 에어로졸 복사강제력이 맑은 날에 비해 3~4배 정도 크게 나타났다. 4월 14일과 16일에의 대기복사가열률 (${\Delta}H$)는 $1{\sim}2\;K\;day^{-1}$ 범위에서 산출되었으며, 4월 15일과 4월 17~18일에는 MPL 관측에서 보여지는 에어로졸층에서의 ${\Delta}H$와 ${\Delta}H_{aerosol}$가 각각 $3\;K\;day^{-1}$ 이상과 $1{\sim}3\;K\;day^{-1}$ 범위에서 산정되었다. 에어로졸 광학적 두께와 비대칭 변수의 변화에 따른 에어로졸층의 ${\Delta}H$ 변화는 미미하였으나, 단산란 알베도의 10% 변화는 지표면과 대기상단에서의 에어로졸 직접복사강제력의 30%, 대기복사강제력의 약 60%, 그리고 에어로졸층 ${\Delta}H$의 약 35% 변화를 유발하였다. 이는 에어로졸 광학적 두께 10% 변화와 비교하여 대기흡수 또는 에어로졸층의 가열 및 냉각 효과가 6배 가량 큰 결과로, 태양복사를 효과적으로 잘 흡수하는 에어로졸의 양에 의해 대기 가열 또는 ${\Delta}H$가 크게 좌우됨을 의미한다. 2001년 4월부터 2008년 3월까지 제주 고산기후관측소에서의 AERONET sun/sky radiometer 관측 자료를 이용하여 계산한 ${\Delta}H$와 ${\Delta}H_{aerosol}$의 월변화를 보면, ${\Delta}H$는 4~8월 사이에 대류권 하부에서 약 $1.0\;K\;day^{-1}$ 이상으로 뚜렷하게 나타났으나, ${\Delta}H_{aerosol}$의 경우 2월부터 6월까지 고도 2 km 이하에서 약 $0.8\;K\;day^{-1}$ 이하의 범위에서 나타나는데, 이는 대부분의 에어로졸이 지표면 부근의 대기경계층에 존재하며, 봄철 황사와 오염 에어로졸의 증가에 의한 영향으로 판단된다.

• Journal of Mechanical Science and Technology
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• 제15권2호
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• pp.239-247
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• 2001

Measured radiative heat fluxes on the furnace exit plane of a heavy duty power boiler of steam output 1650 T/h are discussed. A high-ash pulverized bituminous coal was used. Such measurements are necessary to improve heat fluxes inside a steam boiler furnace was manufactured. An extra small heat radiation sensor was placed in the water cooled head of the probe. The sensor had no direct contact with furnace gases and measured only the radiant energy. There was no exposure to convective heat transfer. With the radiometric probe, one can obtain a spherical indicatrix of radiation intensity as well as hemispherical radiative heat flux incident on any surface passing through a measuring point inside the furnace. Thus, the quantity of radiation energy, passing through the furnace exit plane, to the convective heating surfaces and the quantity of radiation energy going in the opposite direction were measured. A formula for relative radiative heat flux on the furnace exit plane has been proposed.

• 설비공학논문집
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• 제25권5호
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• pp.289-296
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• 2013

A near infrared (NIR) heating system has advantages over the conventional convection-based systems, in terms of heating uniformity and energy efficiency. When it is over-heated during its operation, the radiation lamp gets blackened, and the life of the radiation module becomes severely limited. The heat transfer system in the module is based on a high operating-temperature, and the radiation makes it difficult to analyze in detail the reliability issue, with an experimental approach alone. We developed a numerical heat-transfer model of the NIR heating system. We applied a ray-tracing method on the radiative heat transport, and a finite volume method on the conductive and convective systems, respectively. The cooling performance of the system is presented, based on the energy and flow distributions in the module. The factors that directly affect the module life are analyzed, such as the surface temperatures of the lamp glass and the reflector, and design improvements are discussed.