• 융합정보논문지
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• 제7권5호
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• pp.53-58
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• 2017

석유 고갈의 시대에 저가이면서 반투명한 특징을 갖고 있는 염료감응형 태양전지(DSC)는 1991년 $Gr{\ddot{a}}tzel$의 연구결과 보고 이후 많은 주목을 받아왔다. 염료감응형 태양전지의 광전극의 빛 수확 성능을 증진시키고, 궁극적으로 광전변환효율을 향상시키기 위하여 다양한 구조를 갖는 산란층이 광전극 소재로 제안되었다. DSC 광전극의 산란층에서 산란의 중심으로는 지름이 250 - 300 nm 정도의 크기를 갖는 비교적 큰 이산화티탄 나노입자가 필요하다. 본 연구에서는 변형된 졸겔 공정을 이용하여 약 300 nm 크기의 이산화티탄 나노결정을 합성하였다. XRD와 TEM 분석결과에 의하면, 합성된 이산화티탄 나노입자는 아나타제 상의 단결정 특성을 나타내었다. 합성된 이산화티탄 나노입자를 이용하여 스핀 코팅 공정으로 제조된 이산화티탄 박막의 광학적 투과율은 550 nm 파장에서 약 50%로 측정되었다. 이처럼 적당한 투과율은 DSC 산란층의 산란 중심으로 사용하기에 적합하며, DSC의 광전변환효율 향상에 적절하게 기여할 것으로 기대된다.

• 천문학회보
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• 제37권2호
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• pp.115.2-115.2
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• 2012

In this study we have used the data of various instruments onboard the THEMIS spacecraft to study the characteristics of the outer radiation belt during the ascending phase of solar cycle 24. The most astonishing result is that we discovered four long-term (a month or so) periods during which the belt has nearly disappeared. The first disappearance started late 2008, followed by reappearance in ~a month, and three more similar events repeated until early 2010 when the belt has reappeared. This is well revealed at 719 keV electrons, which is the currently available uppermost energy channel from the THEMIS SST observation, but also seen at even lower energies. Overall consistent features were confirmed using the NOAA-POES observations. The vanished belt periods are associated with extremely weak solar wind conditions, low geomagnetic disturbances (in terms of Kp and AE/AL), greatly suppressed wave (ULF and chorus) activities, greatly reduced storm and substorm activities (little source particle supply), and expanded plasmapause locations. The direct observations of such events shed light on the fundamental question of the origin of the radiation belt, which is the main focus of our presentation.

• 한국태양에너지학회 논문집
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• 제22권3호
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• pp.47-56
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• 2002

The office is an excellent candidate for implementing daylighting techniques because of the relatively high electric lighting power densities and long daytime use pattern. The quantity of light available for a space can be translated in term of the amount of energy savings through a process of a building energy simulation. To get significant energy savings in general illumination, the electric lighting system must be incorporated with a daylight - activated dimmer control. A prototype configuration of an office interior has been established and the integration between the building envelope and lighting and HVAC systems is evaluated based on computer modeling of a lighting control facility. First of all, an energy-efficient luminaire system is designed for both a totally open-plan office interior and a partitioned office. A lighting design and analysis program, Lumen-Micro 2000 predicts the optimal layout of a conventional fluorescent lighting fixture to meet the designed lighting level and calculates unit power density, which translates the demanded amount of electric lighting energy. A dimming control system integrated with the contribution of daylighting has been applied to the operating of the artificial lighting. Annual cooling load due to lighting and the projecting saving amount of cooling load due to daylighting under overcast diffuse sky are evaluated by a computer software, ENER-Win. In brief, the results from building energy simulation with measured daylight illumination levels and the performance of lighting control system indicate that daylighting can save over 70 percent of the required energy for general illumination in the perimeter zones through the year. A 25 % of electric energy for cooling may be saved by dimming and turning off the luminaires in the perimeter zones.

• 한국태양에너지학회 논문집
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• 제35권3호
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• pp.27-39
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• 2015

Under the goal of analyzing the compulsory supply share of new renewable energy according to the application of a daylighting system to indoor gymnasiums, this study conducted analysis of energy consumption and operation schedule at three indoor gymnasiums in the nation through a survey. The investigator did an Energy Plus simulation on Building A based on the analysis results and analyzed the supply share of new renewable energy in the saving effects of lighting energy according to the application of a daylighting system. As a result, When 92 prism daylighting system were installed in the upper ceiling of a stadium, they were able to meet the criteria for the minimum illumination for official games(Min : 600㏓) and optimum illumination for general games and recreations, thus saving lighting energy during the daytime(09:00~17:00). The resulting saving effects of lighting energy amounted to 44.4% for official games, 57.6% for general games, and 66.7% for recreations. In addition, the daylighting systems had a compulsory supply share of new renewable energy at 2.04% for official games, 2.75% for general games, and 2.62% for recreations, recording an average compulsory supply share of 2.5%.

• 대한화장품학회지
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• 제26권1호
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• pp.41-58
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• 2000

최근 환경오염으로 인한 지구오존층의 파괴로 자외선의 지표면의 도달 량이 증가하고 그로 인한 인간에 대한 피해가 증가하고 있다 . 과도한 자외선의 피부에 대한 직접적인 노출은 피부에 많은 문제점을 야기하므로 일차적으로 자외선차단제를 이용하여 인체에 대한 직접적인 피해를 최소화 해야한다 . 현재 자외선 차단제는 유기자외선흡수제와 무기자외선산란제가 많이 사용이 되는데 적은량으로도 효과가 높은 유기자외선차단제는 사용 시 주의를 요하므로 국가별로 사용량과 사용여부에 대하여 규제를 하고 있다. 본 연구에서는 플라보노이드류 ,알카로이드류 같은 자외선 흡수 성분을 함유한 식물중 UV/vis spectrophotometer 에서 자외선 흡수 peak을 나타내는 금은화 , 포공영, 녹차 , 황금추출물을 이용하여 화장품의 자외선 흡수제로서의 사용가능성여부를 조사하였다. 또한 식물추출물이 가진 자극성 성분과 오염성, 그들이 가진 유효성분들을 보호하고자 실리콘을 이용한 겔화를 시도하였다 . 자연친화적인 천연물로써 식물추출성분을 이용 유기자외선흡수제의 사용량을 줄이는 자외선홉수보조제로서 가능성을 보여주었다.

• 공업화학
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• 제32권2호
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• pp.125-131
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• 2021

일반적인 반도체 기반의 광촉매는 물질 고유의 밴드갭 때문에 자외선이나 가시광선에 의해서만 활성화될 수 있고, 태양광 에너지의 약 50%를 차지하는 근적외선 영역의 에너지는 활용할 수 없다. 따라서 기존의 반도체 광촉매의 성능을 향상시키기 위해서는 자외선에서 근적외선에 이르는 넓은 영역에서 더 많은 태양광 에너지를 활용할 수 있어야 한다. 태양광의 근적외선 영역을 활용하기 위해 기존 반도체 광촉매를 업컨버전 나노입자와 결합하는 연구들이 수행되고 있다. 업컨버전 나노입자는 근적외선 광자를 여러 개 흡수하여 자외선이나 가시광선으로 변환하여 광촉매를 활성화할 수 있다. 그리고 반도체 광촉매와 업컨버전 나노입자에 플라즈모닉 금속 나노입자를 함께 결합시키면 태양광에 의한 광촉매 활성을 더욱 향상시킬 수 있다. 본 총설은 업컨버전 나노입자를 이용하여 근적외선 영역의 태양광 에너지가 광촉매의 성능 향상에 기여할 수 있도록 하는 최근의 연구결과를 바탕으로 서술하였다.

• 한국전자통신학회논문지
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• 제16권6호
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• pp.1349-1354
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• 2021

일체형 등명기는 운항 중인 선박의 항로 선위를 결정하기 위한 등화장치이다. 현재 태양광을 기반으로 하는 일체형 등명기는 태양광의 일조시간에 따른 제약에 따라 전력 공급의 부족으로 항로 표시 가능한 능력이 제한적이다. 본 논문에서는 해상의 풍부한 전력원인 태양광과 풍력을 동시에 사용하는 신재생에너지 일체형 9해리 LED 등명기를 구축하고 원격 스마트 모니터링 시스템을 구현하였다. 또한 LED 등명기 장치와 모니터링 시스템을 IoT화 함으로서 등명기의 원격제어 가능한 스마트 제어시스템을 마련하였다. 본 원격 스마트 모니터링 시스템을 적용하여 실시간 상태 모니터링 및 원격제어가 가능하게 하여 선박이 안전한 항해를 할 수 있고 등명기 기능의 정확성 및 영속성을 유지하여 해양사고 예방과 사회적 비용을 절감할 수 있다.

• 한국재료학회지
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• 제32권10호
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• pp.419-424
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• 2022

Halide perovskite solar cells (PSCs) have improved rapidly over the past few years, and research on the optoelectrical properties of halide perovskite thin films has grown as well. Among the characterization techniques, photoluminescence (PL), a method of collecting emitted photons to evaluate the properties of materials, is widely applied to evaluate improvements in the performance of PSCs. However, since only photons emitted from the film in the escape cone are included, the photons collected in PL are a small fraction of the total photons emitted from the film. Unlike PSCs power conversion efficiency, PL measuring methods have not been standardized, and have been evaluated in a variety of ways. Thus, an in-depth study is needed of the methods used to evaluate materials using PL spectra. In this study, we examined the PL spectra of the perovskite light harvesting layer with different measurement protocols and analyzed the features. As the incident angle changed, different spectra were observed, indicating that the PL emission spectrum can depend on the measuring method, not the material. We found the intensity and energy of the PL spectra changes were due to the path of the emitted photons. Also, we found that the PL of halide perovskite thin films generally contains limited information. To solve this problem, the emitted photons should be collected using an integrating sphere. The results of this study suggest that the emission spectrum of halide perovskite films should be carefully interpreted in accordance with PL measuring method, since PL data is mostly affected by the method.

• 천문학회보
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• 제46권1호
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• pp.44.2-45
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• 2021

As implied by the zodiacal light and spacecraft impact measurements, the space between large bodies in our Solar System is filled with interplanetary dust particles (IDPs). IDPs give us deeper insight into the composition and evolution of the Solar System, as well as being a crucial reference for extrasolar research. IDPs can be interpreted as bearers of carbon and organic materials, and thus, their interaction with Earth can be considered as important factors for the birth of terrestrial life. One of the key routes of IDPs entering Earth is via meteoroid streams (Love and Brownlee 1993). The Geminid meteoroid stream is a notable example. Together with its source asteroid (3200) Phaethon, the Phaethon-Geminid stream complex (PGC) (Whipple 1983; Gustafson 1989) can potentially provide information on the properties and evolution of IDPs in near-Earth space. DESTINY+* is a JAXA/ISAS spacecraft planned to launch in 2024 to explore the physical and chemical features of near-Earth IDPs and uncover the dust ejection mechanism of active near-Earth asteroids, especially Phaethon (Arai et al. 2018). Previous studies on the dust ejection mechanism of Phaethon have various degrees of success in explaining the ejection of submillimeter particles and try to recreate the dust replenishment rate of the Geminid stream. However, none of them are satisfactory for explaining the observed Geminid stream, especially for larger particles of a millimeter and centimeter scales. Inspired by the discovery of rotational mass shedding in the Main Belt region (Jewitt et al., 2014), we investigate a dust ejection scenario by rotational instability on Phaethon. Using the N-body integrator MERCURY6 (Chambers 1999; modified by Jeong 2014), we performed a long-term integration of dust particles of various sizes ejected at ~1 m/s. Through this process, we discuss the implications Phaethon's rotation may have on its ejection, the formation and evolution of IDP by this mechanism, and contribute to the DESTINY+ mission.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권2호
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• pp.38.1-38.1
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• 2009

In this paper we present the first results of summer-time F region irregularities during low solar condition observed using the Gadanki MST radar. Echoes were observed on all 20 nights of radar observations and were mostly confined to the post-midnight hours. Echo morphology is very different from the equinoxial post-sunset plume-like features reported earlier from Gadanki. Echo SNRs are lower by 25 dB than their equinoxial post-sunset counterpart, and are quite comparable to the equinoxial irregularities in the post-midnight hours, which are essentially the decaying post-sunset irregularities. The Doppler velocities, which lie in the range of $\pm$ 100 m s-1, show upward/northward motion of the irregularities during the initial phase in contrast to the observed predominant downward/southward velocities associated with the decaying equinoxial post-midnight F region irregularities. Spectral widths of the summer echoes, which are well below 50 m s-1 and are very similar to those of the decaying equinoxial irregularities, represent the presence of weak plasma turbulence. Simultaneous observations made using a collocated ionosonde show no ionogram trace during 2200-0530 LT except for a few occasions. Weak frequency type spread F observed during midnight hours occurred without prior occurrence of range spread F. Concurrent ionosonde observations made from magnetic equatorial location Trivandrum also show very similar result and thus no height rise of the F layer during the midnight hours could be monitored. The preliminary analysis suggests that the post-midnight irregularities reported here are mostly freshly generated ones. The observations are discussed in the light of other observational results reported earlier and the current under standing on the post-midnight occurrence F region irregularities in summer.