• New Physics: Sae Mulli
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• v.68 no.11
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• pp.1268-1274
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• 2018

Aircraft-warning lights are lights that are used to inform pilots in flight about the presence of buildings or dangerous objects. Currently, the light sources of most aircraft-warning lights have been replaced by light-emitting diodes (LEDs). However, the aircraft-warning lights that are installed do not meet the optical performance standards and may cause airplane collisions. Therefore, the use of such light poses a risk to aviation safety. In order to solve this problem, we designed a Fresnel lens with the same luminous intensity distribution ovef $360^{\circ}$ direction; thus, we collimated the light beam from the LED light source with a narrow beam divergence angle in the form of an array of aspheric pieces. After that, we designed and simulated an aircraft-warning-light optical system with a center luminous intensity of 20,000 cd and a vertical divergence angle of $3^{\circ}$ or more by optimizing the lens' tilt and the distance between the LED and the Fresnel lens.

• Journal of Astronomy and Space Sciences
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• v.16 no.2
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• pp.227-240
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• 1999

We performed CCD photometric observations of W UMa type contact binary BV Dra during eight nights from May 1996 to June 1999 using 61cm telescope at Sobaeksan Optical Astronomy Observatory, and completed BV R light curves of the system. From our observations, we derived nine new times of minimum lights (five timings for primary eclipse, four for secondary) and determined new light elements with the times of minima observed since 1999. Our BV R light curves and Batten & Lu(1986)'s radial-velocity ones were simultaneously analyzed with contact mode (Mode 3) of Wilson-Devinney's binary model, and the photometric and spectroscopic solutions for BV Dra were solved. In the analysis, we derived the solutions of 1999 light curves with and without spots, respectively. As the results, asymmetry of light curves may be interpreted as produced by the existence of two spots; hot spot on the secondary and cool on the primary. Combining solutions of light curves and radial-velocity ones, absolute dimensions of BV Dra are $M_1=0.40M_{odot}$, $M_2=1.01M_{odot}$, $R_1=0.72R_{odot}$, $R_2=0.40R_{odot}$. In mass-radius diagram, the less massive and hotter primary component of BV Dra is near TAMS and the secondary is near ZAMS, which is very similar to the other W-type W UMa binaries.

• The Magazine of the Society of Air-Conditioning and Refrigerating Engineers of Korea
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• v.30 no.4
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• pp.56-60
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• 2001

경험에 의하면 앞에서 언급한 장비의 사용, 규율, 규제된 용제의 사용, 기름 페인트 사용의 억제, 그리고 엄격한 페인트 과정을 따르는 것에 의해 잠수함내의 탄화수소 농도를 100만분의 1 또는 2 수준으로 유지할 수 있다. 예방책으로는 세심한 관찰, 선체내로 들여오는 모든 물질의 기록 그리고 규제된 물질의 사용 시간, 장소 및 양의 제어이다. 이러한 점들은 잠수함 내부를 안전하고 건강한 환경으로 설계하기 위하여 활용될 수 있는 자료들이다. 잠수함 내의 공기질은 적외선 분광 광도계, 질량 분광계, 상자성(paramagnetics), 열전도율, 광이온화 그리고 열량 검사에 의해 분석될 수 있다. 분석된 결과는 과거의 데이터와 비교되어 활성탄충의 교체등을 포함하여 유지 관리의 자료로 활용된다. 이러한 원리를 이용한 다양한 계측기가 선체 내의 대기 상태를 분석하기 위하여 사용된다. 중앙 대기 측정기, 추적 가스 분석기, 수소 탐지기, 이동형 대기 모니터, 이동형 산소 분석기, 탄광 안전 지시계, 열량 분석관, 탐지 펌프 시험기가 사용된다. 이러한 계측기는 잠수 전 또는 후에 사용된다. 계측기는 화재 발생시 영향을 받지 않은 공간 또는 냉매가 충전되는 장소에 사용된다. 오늘날 여러 종류의 특별한 잠수함이 존재한다. 정찰 업무를 통해 세계 평화를 유지하고 특별한 임무를 수행하는 것보다 덜 복잡한 목적을 지닌 잠수함도 있다. 그러나 선원들이 안전한 내부 환경 속에서 바다 속을 항해하고 계속 그 응용 범위를 확장하기 위하여 앞에서 언급한 장비들 또는 그 변형들이 사용되어야 한다.

• Korean Journal of Optics and Photonics
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• v.17 no.1
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• pp.54-59
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• 2006

Biophotonic sensors based on polymer waveguide with Bragg reflection grating are demonstrated in this work. Waveguide Bragg reflectors were designed by using the effective index method and the transmission matrix method. The grating pattern was formed by exposing the laser interference pattern on a photoresist. On top of the inverted rib waveguide, the Bragg reflection grating was inscribed by the O2 plasma etching. In order to perform the bio-molecule detection experiment, a calixarene molecule was self-assembled on top of thin Au film deposited on the waveguide Bragg reflector. To measure the response of the sensor, several PBS solutions with different concentrations of potassium ion from 1 pM to $100\;{\mu}M$ were dropped on the sensor surface. The shift of Bragg reflection wavelength was observed from the fabricated sensor device, which was proportional to the concentration of potassium ion ranging from 1 pM to 108 pM.

• Journal of Dental Rehabilitation and Applied Science
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• v.37 no.4
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• pp.199-208
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• 2021

Purpose: The purpose of this study was to compare and evaluate the masking ability of three types of high translucent zirconia according to the various thicknesses and backgrounds. Materials and Methods: Using three types of high-translucency zirconia (Ceramill zolid fx white, Ceramill zolid ht+ white, Ceramill zolid ht+ preshade A2), 10 cylindrical specimens were fabricated in 10mm diameter and each with four thicknesses (0.6 mm, 1.0 mm, 1.5 mm, 2.0 mm), respectively by CAD/CAM method. The background was 10 mm in diameter and 10 mm in thickness. A1, A2, A3 flowable resin backgrounds, blue-colored core resin background, and Ni-Cr alloy background were prepared, and black, white backgrounds provided by the spectrophotometer manufacturer (x-rite, Koblach, Austria) were used. zirconia specimens and the background specimen were stacked to measure L, a^*, b^* with Spectrophotometer (Color i5, x-rite, Koblach, Austria) and the ΔE value with the other background is calculated. The Calculated mean ΔE values were compared based on perceptibility threshold 1.0 and acceptability threshold 3.7. Nonparametric tests such as Kruskal-Wallis test were performed to verify statistical significance (α = 0.05). Results: There was a significant difference in the mean ΔE value according to the zirconia type, background and thickness change (P = 0.000). Conclusion: According to the results of this study, the pre-colored high-translucent zirconia can obtain the desired zirconia shade when it is restored on teeth, composite resins, and abutments except for the blue resin core.

• Proceedings of the Optical Society of Korea Conference
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• 2003.07a
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• pp.280-281
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• 2003

광도 측정의 기본단위인 칸델라 눈금을 확립하는 방법에는 흑체에서 방출되는 분광복사휘도를 기준으로 사용하는 광원 기반 방법과 극저온 절대 복사계(absolute cryogenic radiometer； ACR)로 부터 출발하여 실현하는 검출기 기반의 두 가지 방법이 사용된다. ACR를 사용하면서 검출기 기반 칸델라 눈금의 불확도가 흑체의 온도 측정 불확도로부터 전파되는 불확도 보다 휠씬 작기 때문에 각국의 국가 측정 표준 대표기관에서 검출기 기반 칸텔라 눈금을 실현하고, 교정이나 측정 서비스를 제공하고 있다. (중략)

• Proceedings of the Optical Society of Korea Conference
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• 2007.02a
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• pp.233-234
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• 2007

• Proceedings of the Optical Society of Korea Conference
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• 2004.02a
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• pp.318-319
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• 2004

• Publications of The Korean Astronomical Society
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• v.7 no.1
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• pp.167-188
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• 1992

서울대 천문학과(SNU)의 Washington 측광계를 사용하여 관측한 자료와 ADC (Astronomical Data Center)의 자료를 분석함으로써 SNU Washington 측광계를 표준화 시켰다. SNU Washington 측광계중에서 C필터에 나타나는 적색광 누출은 V필터와의 결합을 통해 보정했으며, 그 최대값은 K0형에서 약 $0^{m}.14$까지 이른다. ADC의 자료분석 결과 G. K형 별들에 대해 중원소 측광지수와 중원소함량과 서로 잘 일치함을 알 수 있었고. 주계열성의 경우 온도 측광지수와 온도와는 좋은 관계를 보임을 알 수 있었다. 또한 ($M-T_2$)과 ($M-T_1$) 평면상에서는 중원소함량과 광도계급에 무관한 좋은 온도관계를 나타냄을 알았다. 그리고 이 측광계의 장점으로 나타난 CN지수와 CN 특이성과는 특별한 관계를 찾기가 어려웠고, 이 측광계만으로는 상도계급의 구분을 다른 측광계 만큼 분명하게 결정짓기가 어려웠다. 그러나 표면중력과이 측광계의 색지수와의 관계를 본 결과 초거성, 거성, 주계열성을 비교적 잘 구분해 낼 수 있었다.

• Transactions of the Korean Society of Mechanical Engineers B
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• v.20 no.11
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• pp.3666-3675
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• 1996

A new hardware temperature compensation method for hot-wire anemometer is investigated and an analog compensating circuit is proposed in this article. A photoconductive cell is introduced here as a variable resistor in the anemometer bridge and the linearized output of a thermistor is used to monitor the input of the photoconductive cell. In contrast with the conventional method, any type of temperature sensor can be used for compensation if once the output of thermometer varies linearly with temperature. So the present technique can diversify the compensating means from a conventional passive compensating resistance to currently available thermometers. Because the resistance of a photoconductive cell can be set precisely by adopting a stabilizing circuit whose operation is based on the integration function of the operational amplifier, the accuracy of compensation can be enhanced. As an example of linearized thermometer, thermistor sensor whose output is linearized by a series resistor was used to monitor the fluid temperature variation. Validation experiment is conducted in the temperature ranged from 30 deg. C to 60 deg. C and the velocity up to 40 m/s. It is found that the present technique can be adopted as a compensating circuit for anemometer and hot-wire type airflow meter.