• KIEAE Journal
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• 제10권3호
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• pp.43-50
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• 2010

Natural lighting is directly connected with our mental and physical health. For working or learning effect, the proper natural lighting is required for improving our living conditions. School facilities, especially, are the place where includes students' ordinary activities with learning behaviors during the school years from elementary to high school. This study was carried out for the purpose introducing a basic database in that planning a school by researching on the actual in the natural lighting system of some schools' classroom, estimating, and analyzing through a simulation, which resulted in a method of improving the natural lighting system. As a result of measuring and analyzing Daylight Factor(DF) during the time from 9 am to 3 pm when students are activating in their classroom, generally DF range of the sides near to window and aisle seats zone are not distributed well. Besides, two out of four school which are researched would not reach the standards of the law for school sanitary while rest of the schools meet the standards; Average DF 5% and Minimum DF 2%. And the result of a simulation by RADIANCE program shows the most appropriate DF range when it is applied in variable numbers about an oriehows the- South-east 15, south-east 30, south-east 45, south-west 15, south-west 30, and south-west 45 degrees. When it is applied in the variable numbers about glass transmittance - 60%, 70%, and 80% in condition facing south of a classroom, the result shows that the DF range of 80% transmittance is relatively higher than other glasses in the classroom. Thus, when a school is built, plans for an orientation is necessary for improve of elementary schools' environment with the glass installation which is made for high transmittance and is regarded with the students' activities time.

• KIEAE Journal
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• 제16권3호
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• pp.25-34
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• 2016

Purpose: The temperature in Seoul has risen 3 times more than the average global temperature increase for the past 100 years. Today, summer starts 15 days earlier than the early 20th century and is 32 days longer. This tendency causes rapid increase of cooling energy demand. Following this effect, seawater heat resources are to be used as an countermeasure for global warming. Incheon Port near the Western Sea has the lowest water temperature in the winter in South Korea in which it is suitable to use seawater cold heat resources. Method: The cold heat resource is gained from seawater when the water temperature is the lowest in the winter time and saved in a seasonal thermal storage. This can be used as cold heat resource in the summer time. A heat exchanger is essential to gain seawater cold energy. Due to this necessity, sea water heat resource heat exchangers are modeled by heat transfer equations and the fluid characteristics are analyzed. Also, a CFD (computational fluid dynamics) program is used to conduct simulation on the fluid characteristics of heat exchangers. The analyzed data of deducted from this process are comprehensively analyzed and discussed. Result: Regarding the performance of the heat exchanger, the heat exchanger was operated following the prediction within the range of heat transfer rate of minimum 3.3KW to maximum 33.6KW per device. In the temperature change analysis of the heat exchanger, fluid analysis by heat transfer equations almost corresponded to the temperature change by CFD simulation. Therefore, it is considered that the results of this study can be used as design data of heat exchangers.

• 천문학회지
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• 제47권6호
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• pp.293-302
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• 2014

Simultaneous time monitoring observations of $H_2O$ $6_{16}-5_{23}$, SiO J = 1-0, 2-1, 3-2, and $^{29}SiO$ ${\upsilon}=0$, J = 1-0 lines are carried out in the direction of the Mira variable star TX Cam with the Korean VLBI Network single dish radio telescopes. For the first time, the $H_2O$ maser emission from TX Cam is detected near the stellar velocity at five epochs from April 10, 2013 (${\phi}=3.13$) to June 4, 2014 (${\phi}=3.89$) including minimum optical phases. The intensities of $H_2O$ masers are very weak compared to SiO masers. The variation of peak antenna temperature ratios among SiO ${\upsilon}=1$, J = 1-0, J = 2-1, and J = 3-2 masers is investigated according to their phases. The shift of peak velocities of $H_2O$ and SiO masers with respect to the stellar velocity is also investigated according to observed optical phases. The $H_2O$ maser emission occurs around the stellar velocity during our monitoring interval. On the other hand, the peak velocities of SiO masers show a spread compared to the stellar velocity. The peak velocities of SiO J = 2-1, and J = 3-2 masers show a smaller spread with respect to the stellar velocity than those of SiO J = 1-0 masers. These simultaneous observations of multi-frequencies will provide a good constraint for maser pumping models and a good probe for investigating the stellar atmosphere and envelope according to their different excitation conditions.

• 대한기계학회논문집B
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• 제29권5호
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• pp.643-652
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• 2005

Saturated nucleate pool boiling experiments for binary mixtures, which are consisted of refrigerant R11 and R113, were performed with constant wall temperature condition. Results for binary mixtures were also compared with pure fluids. A microscale heater array and Wheatstone bridge circuits were used to maintain the constant temperature of the heating surface and to obtain heat flow rate measurements with high temporal and spatial resolutions. Bubble growth images were captured using a high speed CCD camera synchronized with the heat flow rate measurements. The departure time for binary mixtures was longer than that for pure fluids, and binary mixtures had a higher onset of nucleate boiling (ONB) temperature than pure fluids. In the asymptotic growth region, the bubble growth rate was proportional to a value between $t^{\frac{1}{6}}$ and $t^{\frac{1}{4}}$. The bubble growth behavior was analyzed to permit comparisons with binary mixtures and pure fluids at the same scale using dimensionless parameters. There was no discernable difference in the bubble growth behavior between binary mixtures and pure fluids for a given ONB temperature. And the departure radius and time were well predicted within a ${\pm}30{\%}$ error. The minimum heat transfer coefficient of binary mixtures occurred near the maximum ${\mid}y-x{\mid}$ value, and the average required heat flux during bubble growth did not depend on the mass fraction of R11 as more volatile component in binary mixtures. Finally, the results showed that for binary mixtures, a higher ONB temperature had the greatest effect on reducing the heat transfer coefficient.

• 대한방사선기술학회지:방사선기술과학
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• 제8권2호
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• pp.29-45
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• 1985

Computed Tomography Scanner (CT) is highly expensive in operation as well as purchasing. That reason may cause not only to increase the burden of patients but also to waste the capital resources leading to financial difficulties. However the numbers of CT installed throughout the country is increasing, because of efficiency in medical care, patient's concern, competitions among the hospitals within the same area. In the non-Metropolitan area the scanners were expected to be less utilized and less profitable. Nine hospitals equipped with the CT were studied on the utilization of that equipment during the period from November 1984 to February 1985 in non-Metropolitan area and break-even point in one hospital was analyzed for estimating profitabilities. The results were as follows ; 1. Among those nine hospitals, four hospitals had less than 400 beds, which is one of the restrictive minimum standards on the installation of Whole-body Computed Tomography Scanner. 2. The operating time during the normal operation period was longer than those of any other studies, but the accumulated down time was also longer than those of any other studies. The average number of scanning per week for each CT was 45, while the estimated number of for the break-even point was 56.7 cases. 3. When the downtime was excluded in calculating the average operation would be much closer to the cases for the break-even point. Therefore the break-down of the equipment was to be a main cause of the low profitability. 4. The average scanning rate for head area was 33.6%, however three of the nine hospitals showed about 20%. 5. If scanning ratio for the body parts excepting head was increased, the number of scanning for the break-even point would be diminished. 6. The small size hospital especially located near the Metropolitan area showed largest loss in the CT operation. In purchasing the highly expensive equipments in hospitals, demand should be taken into account and planning is recommended.

• 한국위성정보통신학회논문지
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• 제11권2호
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• pp.55-59
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• 2016

기존 무선에너지 하비스팅시스템에서 유저는 하나의 Hybirid-AP (H-AP)로부터 에너지와 정보를 동시에 받았다. 하지만 무선에너지 하비스팅은 거리가 멀수록 감쇄가 심하기 때문에 H-AP에서 거리가 먼 유저들은 낮은 하비스팅 효율 가진다 (이중 근거리/원거리 문제). 이러한 문제를 해결하기 위해서 본 논문은 Power beacon (PB)을 통해 유저에게 별도의 파워를 공급하는 비결합 무선에너지 하비스팅 네트워크를 시스템 모델로 사용하였다. 이 논문의 주된 목적은 다양한 제약 조건과 Quality of service (QoS), 그리고 Quality of harvested power (QoP)를 만족하면서 목적 함수인 Energy efficiency (EE)를 최대화 하는 것이다. 제안된 시스템은 라그랑지안 쌍대 분해법 이론을 기반으로 EE 최대화를 위한 최적의 시간 스케줄링 알고리즘을 제안한다. 이 알고리즘을 통해 프레임 분해 요소, H-AP의 송신파워, 그리고 PB의 송신파워의 최적 값과 EE의 최대값을 구할 수 있다. 모의 실험 결과는 제안된 알고리즘으로 파라미터가 최적 값으로 빠르게 수렴하고 제안된 모델의 성능이 기존의 시스템 모델보다 우수하다는 것을 증명한다.

• 고려인삼학회:학술대회논문집
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• 고려인삼학회 1984년도 학술대회지
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• pp.49-55
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• 1984

미국인삼 1년생근을 재료로 하여 각 온도조건별(-15, 0, 3, 6, 9, 12 및 $15^{\circ}C$)로 120일 이상 온도 처리한 후 온실 조건에 식부하여 성장기간동안 출아 소요일수 및 근중 증가율을 조사하였다. $0^{\circ}C$ 이하와 $9^{\circ}C$ 이상에서도 출아가 되지 않았으며 발아기능 온도 범위내에서는 온도에 따른 출아 소요일은 거의 차이가 없었다. 저장기간이 싹의 후면 타파력 및 휴면타파 종료일로부터 발아일(R = 91)까지의 기간에 큰 영향을 미쳤다. $100{\%}$의 출아를 위해서는 약 1,800시간의 저온 처리가 요구되었다. 720시간의 휴면 타파를 위한 저온 처리를 받은 인삼근의 $15{\%}$가 근관을 형성하였다. 휴면 타파가 출아에 소요되는 총 시간은 저온 처리의 온도와 관계없이 일정하게 거의 125일 (3,000시간) 이었다. 이러한 발견은 인삼재배를 위한 온도 조건을 고려한 적지 판정을 하는데 유용하게 이용될 것이다. 이는 개체군에 따라 휴면 타파를 위한 저온처리 충족요건이 유전적으로 다를 것이라는 사실을 시사해 준다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2008년 영문 학술대회
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• pp.330-339
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• 2008

Ground-based interceptors(GBI) comprise a major element of the strategic defense against hostile targets like Intercontinental Ballistic Missiles(ICBM) and reentry vehicles(RV) dispersed from them. An optimum design of the subsystems is required to increase the performance and reliability of these GBI. Propulsion subsystem design and optimization is the motivation for this effort. This paper describes an effort in which an entire GBI missile system, including a multi-stage solid rocket booster, is considered simultaneously in a Genetic Algorithm(GA) performance optimization process. Single goal, constrained optimization is performed. For specified payload and miss distance, time of flight, the most important component in the optimization process is the booster, for its takeoff weight, time of flight, or a combination of the two. The GBI is assumed to be a multistage missile that uses target location data provided by two ground based RF radar sensors and two low earth orbit(LEO) IR sensors. 3Dimensional model is developed for a multistage target with a boost phase acceleration profile that depends on total mass, propellant mass and the specific impulse in the gravity field. The monostatic radar cross section (RCS) data of a three stage ICBM is used. For preliminary design, GBI is assumed to have a fixed initial position from the target launch point and zero launch delay. GBI carries the Kill Vehicle(KV) to an optimal position in space to allow it to complete the intercept. The objective is to design and optimize the propulsion system for the GBI that will fulfill mission requirements and objectives. The KV weight and volume requirements are specified in the problem definition before the optimization is computed. We have considered only continuous design variables, while considering discrete variables as input. Though the number of stages should also be one of the design variables, however, in this paper it is fixed as three. The elite solution from GA is passed on to(Sequential Quadratic Programming) SQP as near optimal guess. The SQP then performs local convergence to identify the minimum mass of the GBI. The performance of the three staged GBI is validated using a ballistic missile intercept scenario modeled in Matlab/SIMULINK.

• 대한토목학회논문집
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• 제42권1호
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• pp.23-33
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• 2022

상시미동의 수직성분에 대한 수평성분 스펙트럼비(HVSR)는 부지 공명주파수를 파악하는데 활발히 사용되고 있다. HVSR의 가장 큰 비율을 가지는 주파수는 부지 공명주파수와 일치한다. 상시미동은 부지 주변에 존재하는 미세진동을 의미하기 때문에 직접적인 진동원을 파악할 수 없으며, 또한 조절할 수 없다. 따라서 신뢰적인 상시미동 HVSR을 구하기 위해서는 상시미동 측정에 충분한 시간적 여유와 주변 환경의 파악 또한 필요하다. 본 연구에서는 신뢰적인 HVSR 분석에 필요한 상시미동 측정 최소시간과 지진계와 인위적인 진동 사이의 이격거리의 영향을 알아보았다. 토사 부지의 경우 센서 설치 후 5분 이내에 안정화가 되었으나, 암반 부지의 경우 안정화까지 1시간 이상이 소요되었다. 또한 상시미동 관측 시 발걸음 진동이 지진계 10 m 이내에 존재할 경우 HVSR결과에 큰 영향을 미치는 것을 확인하였다. 이러한 결과는 현장에서 상시미동의 HVSR측정에 필요한 가이드라인을 제공할 것으로 기대된다.

• 한국화재소방학회논문지
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• 제13권1호
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• pp.37-47
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• 1999

부유중인 분진의 화재 및 용기 또는 파이프의 미세한 균열에서 비산되는 가연성 액체의 분무화재의 위험성은 착화후의 고속 확산과 높은 열방출율로 인하여 매우 높은 것으로 알려졌다. 이에 대한 연구는 주로 실험적으로나 또는 거시적인 관점의 해석으로 제한되어 왔다. 본 연구는 미시적인 관점의 해석으로서 분진 및 분무를 가연성 미세 액적으로 가정하여 그의 증발과 착화에 대하여 연구하였다. 첫 단계로서 일열의 액적 배열을 계산영역으로 하여, 비정상 이차원 보존방정식들을 적용하였다. 수치해석은 일반화된 비직교 좌표계를 사용하였고, 화학반응은 Arrhenius의 법칙에 의하여 반응속도가 제어되는 일단계 반응을 고려하였다. 계산결과는 액적 주위의 온도와 반응물질의 농도분포를 시간에 따라 보여준다. 주위의 산소가 증발하는 액적의 연료와 섞이기 시작하고 착화 조건에 다다르면, 급격한 발열반응이 예혼합된 가스로부터 일어나기 시작한다. 최대온도 영역은 점차적으로 액적 표면으로 이동하며 최대온도는 착화이후 급격히 상승한다. 연료와 산소의 농도는 최대온도 영역 근처에서 최소값을 보인다. 따라서 착화순간에는 예혼합연소의 양상을 띠는 것으로 나타났다. 이후에는 예혼합 가스의 소멸로 확산연소의 양상을 띠게 된다. 액적간의 거리는 중요한 요소로서 멀리 떨어져 있는 경우부터 액적간의 거리가 가까워지면 착화지연 시간이 줄여들어 착화가 빨리 일어나는 것으로 관찰되었다. 또한 착화 후에는 최대온도 영역이 일열의 중심선으로부터 멀어지는 것으로 나타났는데 이것은 중심부근의 산소가 먼저 소모되고 외부로부터의 산소공급도 화염에 의해 차단되어 나타나는 현상이다. 이번 연구로 미세적인 착화현상에 대한 이해를 높이게 되었고 추후 복잡한 배열에 대한 연구도 가능할 것이다.