• Transactions on Electrical and Electronic Materials
• /
• 제16권4호
• /
• pp.201-205
• /
• 2015

This paper dealt with the condensing technology of an LED light source that uses a parabolic reflector to replace a searchlight equipped with a xenon lamp. A ray-tracing simulation was conducted to analyze the influence of the diameter of the reflector and the size of the light source on light condensing. The combination of a parabolic reflector with a diameter of 620 mm and a focal distance of 220 mm, and a 9 mm multi-chip package (MCP) with a luminous flux of 7,000 lm showed the narrowest beam angle. The luminous intensity at the center was measured at 7.7×10⁶ cd. The distance between the light source and the point where the illuminance was 1 lx was calculated to be 2.8 km. The power consumption of the system was 95 W, which is only 9.5% of that of the 1 kW xenon searchlight, and the beam angle was 1.03°. In a site experiment, it was confirmed that the light ray reflected from the LED searchlight proceeds forward without any diffusion because of the narrow beam angle.

• Journal of Advanced Marine Engineering and Technology
• /
• 제38권6호
• /
• pp.737-743
• /
• 2014

본 논문에서는 기존 1kW 할로겐 탐조등을 대체하기 위한 고출력 LED 탐조등에 관하여 기술하였다. 설계사양은 KDS 6230-1046-1과 KS V 8469를 기준으로 하였으며, 요구 광도 800,000cd를 만족시키기 위하여 지향각 $6^{\circ}$의 렌즈를 사용하였다. 시제작 LED 탐조등의 방열은 공랭식으로써 팬이나 히트파이프를 사용하지 않았다. 시험결과, 시제작 LED 탐조등의 소비전력은 148W로 1kW 할로겐 탐조등에 비해 85% 절감되었으며, 중심광도는 945,000cd로써 KS V 8469를 만족하였다. 광효율은 기존 탐조등보다 4.7배 향상되었으며, 지향각, 색온도 및 연색성은 각각 $5.4^{\circ}$, 5,500K, 70이었다. LED 탐조등의 외함 온도는 $60^{\circ}C$ 이하이고, SMPS 주변 온도는 $50^{\circ}C$ 이하로 IEC 60092-306을 만족하였다.

• 한국전기전자재료학회논문지
• /
• 제27권9호
• /
• pp.594-599
• /
• 2014

The heat dissipation conditions of high-power 5 watt LEDs-based searchlight modules were optimized with varying LED bar'shape, materials, and ambient temperature. The LED junction temperature was estimated by using Computational Fluid Dynamics simulation. The optimal heat dissipation conditions were found as follows; LED bar' shape: L=80 mm, W=4 mm, t=10 mm, copper material, LED junction temperature of $116.6^{\circ}C$, ambient temperature of $50^{\circ}C$, total mass of 184 g, and shadowing area of $320mm^2$. The difference between the junction temperatures of our fabricated and simulated LEDs-based searchlight modules is about $3^{\circ}C$, which confirms the validity of our thermal simulation results.

• 한국광학회지
• /
• 제31권2호
• /
• pp.81-87
• /
• 2020

본 연구에서는 좁은 지향각, 높은 최대 중심광도를 갖는 탐조등 광학계 설계 기술 연구를 진행하였다. 기존 탐조등 광원인 할로겐램프와 제논램프는 진동과 충격에 취약하며, 크기가 크고 무거워 운반에 많은 어려움이 있다. 또한 탐조등 후면부에 위치한 포물경은 제작 시 광원과 조립 오차에 따른 성능 저하와 낮은 광 효율의 단점을 지니고 있다. 이를 해결하기 위해 본 논문에서는 1 kW 할로겐램프를 150 W급 고출력 COB LED로 대체하고 목표 성능을 만족하기 위한 고효율 TIR 렌즈를 설계하였다. 이후 광학계 사출 시 발생하는 표면 오차를 해결하는 방안으로 TIR 렌즈 어레이를 제시하여 제작 신뢰성을 확보하였다. 설계된 광학계를 바탕으로 시제품을 제작한 후 시중 할로겐램프 탐조등과 성능을 비교하여 광학 성능의 우수함을 확인하였다.

• 한국산학기술학회논문지
• /
• 제19권11호
• /
• pp.332-337
• /
• 2018

항공기용 탐조등은 야간 임무 수행 시 탐색 또는 구조 임무에 사용되며, 은폐 상태를 유지하며 작전을 수행할 수 있도록 적외선 광을 제공한다. A기종 회전익 항공기 운용 중에, 적외선 생성을 위한 적외선 투과 필터 유리가 파손되는 현상이 다수 발생하였으며, 이로 인해 은폐능력이 상실되고 정비 소요가 발생하는 등의 문제점이 제기되었다. 본 논문에서는 해당 결함이 발생하는 탐조등의 운용 조건을 시험하고, 그에 따른 결함 원인을 도출한 과정을 기술하였다. 그리고 도출된 원인을 개선하기 위한 여러 가지 방안과 개선 필터 시제품 제작 과정을 정리하였다. 또한 개선된 필터가 장착된 탐조등에 대해 성능시험, 내구성 시험, 항공기 장착시험을 통해 탐조등의 규격에서 제시하는 성능 요구를 만족하는지 검증한 결과를 기술하였다. 시험 및 검증 결과 필터의 파손 현상이 개선되었으며, A 기종 항공기에 개선 필터를 적용한 결과 파손 현상이 더 이상 발생하지 않는 것을 확인하였다.

• 대한기계학회논문집B
• /
• 제20권11호
• /
• pp.3598-3606
• /
• 1996

The finite volume method for radiation is applied to investigate a radiative heating of rocket base plane due to searchlight and plume emissions. Exhaust plume is assumed to absorb, emit and scatter the radiant energy isotropically as well as anisotropically, while the medium between plume boundary and base plane is cold and nonparticipating. Scattering phase function is modelled by a finite series of Legendre polynomials. After validating benchmark solution by comparison with that of previous works obtained by the Monte-Carlo method, further investigations have been done by changing such various parameters as plume cone angle, scattering albedo, scattering phase function, optical radius and nozzle exit temperature. The results show that the base plane is predominantly heated by the plume emission rather than the searchlight emission when the nozzle exit temperature is the same as that of plume.

• 기술사
• /
• 제34권5호
• /
• pp.40-43
• /
• 2001

상암동 월드컵 주정기장은 축구 전용경기장으로서 2002년 월드컵 축구경기를 위한 꿈과 감동의 라이브 스테이지로서의 스타디움 시설로 각종 국내외 축구경기는 물론 문화행사를 효율적으로 운영할 수 있도록 계획되었다. 이에 효율적인 경기장 시스템 구성과 적정한 전기시설물 설치로 최상의 경기운영을 할 수 있도록 전력시스템을 안정화 하였으며, 월드컵 경기 이후 스포츠공간과 상업시설, 공공시설 등 복합화된 스포츠 문화시설에 부합할 수 있도록 수변전 설비 및 방재센타 등을 다분화하여 시설하였으며 국제적 행사의 장에 전기인으로서 일익을 담당할 수 있었음에 감사한 마음이다.

• KSII Transactions on Internet and Information Systems (TIIS)
• /
• 제12권10호
• /
• pp.4889-4902
• /
• 2018

It is a challenging issue to improve the energy efficiency of neighbor discovery in WSNs. This paper proposes an optimal discovery model (ODM) for the first time. Based on the model, we investigate the influence of the relative size of two unequal active slots on the energy efficiency. ODM provides the energy optimal value of the length of the larger active slot at a given duty cycle. Other than existing methods, the worst-case latency bound of ODM is only one period. This is a subversive conclusion, because almost all other related methods are based on a wake-up schedule that contains several periods. We theoretically deduce that ODM can reduce worst-case discovery latency by 43.89% compared to Searchlight-Trim when their duty cycles are the same. The simulations verify the advantage of ODM.

• International journal of advanced smart convergence
• /
• 제1권2호
• /
• pp.59-63
• /
• 2012

The mVoIP service is the technology which focuses on the wireless data service as the IP network having the transmission rate of 100 Mbps classes on the high-speed middle of movement through the WiFi, WiBro and 3G mobile radio communication network, and etc. and is developed. Since 2010, the mVoIP (mobile VoIP) service shows the rapid growth due to 4G-LTE service seriously disclosed from July with the Smart phone and 2,011 it begins to be rapidly popularized. In this research, additionally the mVoIP service industry activation plan is presented with the trends of technology development including the chip-set/module/terminal, etc. based upon local and foreign market trend searchlight through the market demand analysis. The mVoIP service downloads App to the mobile apparatus and or can provide the service as the software through the WiFi network. Therefore, the change which is large in the products development aspect is to be have no. Expected to is being provided as the added service in the case of 4G-LTE as a matter of course, the service deployment where it is based on the market principle and demand needs is needed.

• 천문학회보
• /
• 제46권2호
• /
• pp.36.1-37
• /
• 2021

Six images of IRC+10216 taken by the Hubble Space Telescope at three epochs in 2001, 2011, and 2016 are compared in the rest frame of the central carbon star. An accurate astrometry has been achieved with the help of Gaia Data Release 2. The positions of the carbon star in the individual epochs are determined using its known proper motion, defining the rest frame of the star. In 2016, a local brightness peak with compact and red nature is detected at the stellar position. A comparison of the color maps between 2016 and 2011 epochs reveals that the reddest spot moved along with the star, suggesting a possibility of its being the dusty material surrounding the carbon star. Relatively red, ambient region is distributed in an Ω shape and well corresponds to the dusty disk previously suggested based on near-infrared polarization observations. In a larger scale, differential proper motion of multiple ring-like pattern in the rest frame of the star is used to derive the average expansion velocity of transverse wind components, resulting in ~12.5 km s-1 (d/123 pc), where d is the distance to IRC+10216. Three dimensional geometry is implied from its comparison with the line-of-sight wind velocity determined from half-widths of submillimeter emission line profiles of abundant molecules. Uneven temporal variations in brightness for different searchlight beams and anisotropic distribution of extended halo are revisited in the context of the stellar light illumination through a porous envelope with postulated longer-term variations for a period of 10 years.