• 설비공학논문집
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• 제18권3호
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• pp.211-217
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• 2006

The three-dimensional numerical analysis has been carried out to figure out the effect of the thermoelectric element thickness on the thermal performance of the thermo-electric micro-cooler. The small-size and column-type thermoelectric cooler is considered. It is known that tellurium compounds currently have the highest cooling performance around the room temperature. Thus, in the present study, $Bi_{2}Te_{3}$ and $Sb_{2}Te_{3}$ are selected as the n- and p-type thermoelectric materials, respectively. The thermoelectric leg considered is less than $20{\mu}m$ thick. The thickness of the leg may affect the thermal and electrical transport through the interfaces between the leg and metal conductors. The effect of the thermoelectric element thickness on the thermal performance of the cooler has been investigated with parameters such as the temperature difference, the current, and the cooling power.

• 제어로봇시스템학회:학술대회논문집
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• 제어로봇시스템학회 2005년도 ICCAS
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• pp.139-144
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• 2005

A rigorous research is underway in our team, for the design and development of high figure of merits (ZT= 1.5${\sim}$2.0) micro-thermoelectric coolers. This paper discusses the fabrication process that we are using for developing the $Sb_2Te_3-Bi_2Te_3$ micro-thermoelectric cooling modules. It describes how to obtain the mechanical properties of the thin film TEC elements and reports the results of an equation-based multiphysics modeling of the micro-TEC modules. In this study the thermoelectric thin films were deposited on Si substrates using co-sputtering method. The physical mechanical properties of the prepared films were measured by nanoindentation testing method while the thermal and electrical properties required for modeling were obtained from existing literature. A finite element model was developed using an equation-based multiphysics modeling by the commercial finite element code FEMLAB. The model was solved for different operating conditions. The temperature and the stress distributions in the P and N elements of the TEC as well as in the metal connector were obtained. The temperature distributions of the system obtained from simulation results showed good agreement with the analytical results existing in literature. In addition, it was found that the maximum stress in the system occurs at the bonding part of the TEC i.e. between the metal connectors and TE elements of the module.

• 한국분말재료학회지
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• 제23권4호
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• pp.263-269
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• 2016

Graphene oxide (GO) powder processed by Hummer's method is mixed with p-type $Bi_2Te_3$ based thermoelectric materials by a high-energy ball milling process. The synthesized GO-dispersed p-type $Bi_2Te_3$ composite powder has a composition of $Bi_{0.5}Sb_{1.5}Te_3$ (BSbT), and the powder is consolidated into composites with different contents of GO powder by using the spark plasma sintering (SPS) process. It is found that the addition of GO powder significantly decreases the thermal conductivity of the pure BSbT material through active phonon scattering at the newly formed interfaces. In addition, the electrical properties of the GO/BSbT composites are degraded by the addition of GO powder except in the case of the 0.1 wt% GO/BSbT composite. It is found that defects on the surface of GO powder hinder the electrical transport properties. As a result, the maximum thermoelectric performance (ZT value of 0.91) is achieved from the 0.1% GO/BSbT composite at 398 K. These results indicate that introducing GO powder into thermoelectric materials is a promising method to achieve enhanced thermoelectric performance due to the reduction in thermal conductivity.

• 자원환경지질
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• 제26권1호
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• pp.41-54
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• 1993

경상분지 남동부에 위치한 울산광산은 석회암을 교대한 전형적인 calcareous skarn강상으로 Fe W광화작용 이외에도 Cu, Pb, Zn, As, Bi, Ni, Co, Cr, Ag, Sn, In, Te, Sb 등이 수반되는 다금속광화작용의 특성을 보여주고 있다. 본 광상은 직립에 가까운 파이프상 광체로 산출되며, 자철석과 함께 북측의 혼펠스와의 경계부근에 회중석이 부분적으로 광염되어 있다. 본 광상의 스카른대는 석회암 및 혼펠스를 교대한 괴상 스카른과 양자를 각기 절단하는 맥상스카른으로 구분된다. 괴상스카른은 석회암 기원의 스카른이 주체를 이루며, 이러한 스카른대는 규회석 스카른, 석류석 스카른, 단사휘석-석류석 스카른, 단사휘석 스카른으로 분류되며, 부분적으로 스카른대 주변부를 따라 거정질 방해석대가 존재하고 있다. 스카른 진화과정은 초기스카른 및 후기스카른의 두 시기로 분류되며, 초기스카른은 prograde한 스카른 생성시기로 초기에는 규회석, Mg-rich 단사휘석, Al-rich garnet가 주로 정출되며 광석광물은 거의 불모한 시기이나, 초기스카른의 말기로 진행됨에 따라 자철석과 회중석이 정출된다. 그리고, 후기스카른의 전반기까지는 Fe-rich 단사휘석, Fe-rich garnet와 함께 자철석 회중석이 연속적으로 정출되었으나, 후기스카른의 중기부터는 Ni, Co, As, Cu, Zn, Fe, Bi 등의 황화광물이 정출되는 다금속광화 작용의 특정을 보인다. 또한, 최후기 열수작용시기에는 섬아연석과 방연석 등의 Base-metal 황화광물이 주로 정출되는 연 아연 광화작용의 양상을 나타낸다. 이러한 각 광화시기별 스카른 광물과 광석광물의 변화양상은 고온의 열수용액이 천부로 유출되는 과정에서 광화용액의 온도가 급격히 떨어진 결과 (telescope)에 기인된 것으로 사료된다.

• Transactions on Electrical and Electronic Materials
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• 제15권1호
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• pp.37-40
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• 2014

A novel memory is reported, in which $Ge_2Sb_2Te_5$ (GST) has been used as a floating gate. The threshold voltage was shifted due to the phase transition of the GST layer, and the hysteretic behavior is opposite to that arising from charge trapping. Finite Element Modeling (FEM) was adapted, and a new simulation program was developed using c-interpreter, in order to analyze the small shift of threshold voltage. The results show that GST undergoes a partial phase transformation during the process of RESET or SET operation. A large $V_{TH}$ shift was observed when the thickness of the GST layer was scaled down from 50 nm to 25 nm. The novel 1 transistor PCM (1TPCM) can achieve a faster write time, maintaining a smaller cell size.

• Korean Chemical Engineering Research
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• 제47권6호
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• pp.715-719
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• 2009

본 연구에서는 DNA 정보를 상변화 물질의 전기저항 변화특성으로 검출할 수 있는 상변화 전극 기판을 개발하였다. 이를 위해 반도체 공정에서 사용하는 Al을 사용하여 전극 기판을 제작하였다. 하지만 주사전자현미경을 이용하여 Al 전극의 단면 상태를 확인해 본 결과 PETEOS(plasma enhanced tetraethyoxysilane) 내에서 보이드(void)가 발생하여 후속공정인 에치백과 세정공정 분위기에 과도하게 노출되어 심하게 손상되어 전극과 PETEOS 사이에 홀(hole)로 변형된다. 이 문제점을 해결하기 위하여 에치백 및 세정 공정을 진행하지 않으면서 $Ge_2Sb_2Te_5$(GST) 박막의 단차피복성(stepcoverage)을 좋게 할 수 있고, 열역학적으로 GST 박막과의 반응성을 고려했을 때 안정적이면서 비저항이 낮은 TiN 재료를 사용하여 상변화 전극 기판을 제작하였다. 주사전자현미경을 통하여 전극의 단면의 상태를 관찰하였으며 TiN 전극과 GST 박막이 정상적으로 연결되어 있는 것을 확인하였다. 또한 저항측정 장비를 사용하여 TiN 상변화 전극 기판 위에 증착된 GST의 비정질과 결정질의 저항을 측정하였고, GST의 비정질과 결정질저항의 차이는 약 1,000배 정도로 신호를 검출하는데 충분함을 확인하였다.

• 천문학회보
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• 제37권1호
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• pp.66.1-66.1
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• 2012

We have developed superconducting mixer receivers for 129 GHz VLBI observation in Korean VLBI Network(KVN). The developed mixer has a radial waveguide probe with simple transmission line LC transformer as a tuning circuit to its 5 series-connected junctions, which can have 125-165 GHz as operation RF frequency. For IF signal path a high impedance quarter-wavelength line connects the probe to one end of symmetric RF chokes. DSB receiver noise of the mixer was about 40 K over 4-6 GHz IF band whereas we achieved about uncorrected SSB noise temperature of 70 K and better than 10 dB IRR in 2SB configuration with 8-10 GHz IF band. Insert-type receiver cartridges using the mixers have been assembled for all three KVN stations. On-site performance summary in commissioning phase is presented.

• 한국분말재료학회지
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• 제17권2호
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• pp.136-141
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• 2010

Bismuth-telluride based $(Bi_{0.2}Sb_{0.8})_2Te_3$ thermoelectric powders were fabricated by two-step planetary milling process which produces bimodal size distribution ranging $400\;nm\;{\sim}\;2\;{\mu}m$. The powders were reduced in hydrogen atmosphere to minimize oxygen contents which cause degradation of thermoelectric performance by decreasing electrical conductivity. Oxygen contents were decreased from 0.48% to 0.25% by the reduction process. In this study, both the as-synthesized and the reduced powders were consolidated by the spark plasma sintering process at $350^{\circ}C$ for 10 min at the heating rate of $100^{\circ}C/min$ and then their thermoelectric properties were investigated. The sintered samples using the reduced p-type thermoelectric powders show 15% lower specific electrical resistivity ($0.8\;m{\Omega}{\cdot}cm$) than those of the as-synthesized powders while Seebeck coefficient and thermal conductivity do not change a lot. The results confirmed that ZT value of thermoelectric performance at room temperature was improved by 15% due to high electric conductivity caused by the controlled oxygen contents present at bismuth telluride materials.

• 한국초전도ㆍ저온공학회논문지
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• 제11권3호
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• pp.65-68
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• 2009

The Stirling cryocoolers have been widely used for the cooling of the infrared detector(InSb, HgCdTe, and etc,) and HTS(High Temperature Superconductor) to the cryogenic temperature. The monobloc Stirling cryocoolers with the rotary compressor are applicable to the cooling device for the compact mobile thermal imaging system, because the cryocoolers have the compact structure and light weight. The typical performance factors of the Stirling cryocooler are the cool-down time, cooling capacity at the desired temperature (80 K), the electric input power and COP. The above performance factors depend on the operating conditions such as the charging pressure of the helium gas, the thermal environment and etc.. In this study, the effects of the thermal environment (temperature of 241, 293, and 333 K) on the performance of the cryocooler were investigated by experiments. The results show the effects of the temperature of the thermal environment on the cooling capacity and input power.

• 천문학회보
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• 제35권1호
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• pp.39.2-39.2
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• 2010

In this paper, I present the domestic development of near infrared camera systems for the ground telescope and the space satellite. These systems are the first infrared instruments made for astronomical observation in Korea. KASINICS (KASI Near Infrared Camera System) was developed to be installed on the 1.8m telescope of the Bohyunsan Optical Astronomy Observatory (BOAO) in Korea. KASINICS is equipped with a $512{\times}512$ InSb array enable L band observations as well as J, H, and Ks bands. The field-of-view of the array is $3.3'{\times}3.3'$ with a resolution of 0.39"/pixel. It employs an Offner relay optical system providing a cold stop to eliminate thermal background emission from the telescope structures. From the test observation, limiting magnitudes are J=17.6, H=17.5, Ks=16.1 and L(narrow)=10.0 mag at a signal-to-noise ratio of 10 in an integration time of 100 s. MIRIS (Multi-purpose InfraRed Imaging System) is the main payload of the STSAT-3 in Korea. MIRIS Space Observation Camera (SOC) covers the observation wavelength from $0.9{\mu}m$ to $2.0{\mu}m$ with a wide field of view $3.67^{\circ}{\times}3.67^{\circ}$. The PICNIC HgCdTe detector in a cold box is cooled down below 100K by a micro Stirling cooler of which cooling capacity is 220mW at 77K. MIRIS SOC adopts passive cooling technique to chill the telescope below 200K by pointing to the deep space (3K). The cooling mechanism employs a radiator, a Winston cone baffle, a thermal shield, MLI of 30 layers, and GFRP pipe support in the system. Opto-mechanical analysis was made in order to estimate and compensate possible stresses from the thermal contraction of mounting parts at cryogenic temperatures. Finite Element Analysis (FEA) of mechanical structure was also conducted to ensure safety and stability in launching environments and in orbit. MIRIS SOC will mainly perform the Galactic plane survey with narrow band filters (Pa $\alpha$ and Pa $\alpha$ continuum) and CIB (Cosmic Infrared Background) observation with wide band filters (I and H) driven by a cryogenic stepping motor.