• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2005년도 춘계학술대회 논문집
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• pp.15-18
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• 2005

As consumer in optics, electronics, aerospace and electronics industry grow, the demand for ultra-precision aspheric surface lens increases higher. To enhance the precision and productivity of ultra precision aspheric surface micro lens, The development of ultra-precision grinding system and manufacturing properties for the aspheric surface micro lens are described. In the work reported in this paper, and ultra-precision grinding system for manufacturing the aspheric surface micro lens was developed by considering the factors affecting the surface roughness and profiles accuracy. And this paper deals with mirror grinding of an aspheric surface micro lens by resin bonded diamond wheel and spherical lens of BK7. It results was that a form accuracy of $3\;{\mu}m$ P-V and a surface roughness of $0.1\;{\mu}m\;R_{max}$.

• 한국정보통신학회:학술대회논문집
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• 한국정보통신학회 2017년도 춘계학술대회
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• pp.463-466
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• 2017

본 논문의 내용은 기존의 차륜식 로봇과는 차별화된 전-방향 구동이 가능한 모듈 개발을 통하여, 기존 모듈의 이동로봇이 가지는 단점인 측면주행성능 저하, 단순 작업주행 경로, 회전-직진 반복 주행으로 인한 불필요한 주행소요시간의 증대 등의 단점을 극복할 수 있을 것이다. 볼-벨런싱 로봇을 구동하기 위한 전-방향 구형휠 구동모듈은 3개의 로터캐스터를 이용한 로봇의 전-방향으로 구동하기 위한 동력전달 메커니즘과 주행을 위한 알고리즘 개발이 요구된다. 3DoF(축) 전-방향 이동 알고리즘이 내장된 드라이버가 모듈에 내장되고, 주행 방향 및 속도를 위한 3DoF(축)의 구동 모터 모듈이 장착된다. 이동 메커니즘으로는 각 구동바퀴의 회전 벡터 합에 따른다. 두 개 또는 세 개의 구동바퀴의 회전과 벡터 합에 따른 다양한 이동방향을 만들어 낼 수 있다. 각 구동바퀴의 회전 벡터장의 여하에 따라 다른 방향으로도 이동이 가능하다. 전-방향 이동을 위한 보다 혁신적인 전-방향 구형휠 구동모듈이 개발되면, 이동로봇의 구동부에 사용되어 로봇의 성능을 기술적으로 좀 더 향상시킬 수 있으며, 구동모듈이 적용된 전-방향로봇 플랫폼을 통하여 기존 차륜식 로봇의 경우 각종 환경에 대한 저항성으로 인해 연속 직진 성능이 저하되는 단점을 극복할 수 있어서 미주, 유럽과 같은 환경에서 적용될 수 있는 청소로봇, 이동로봇뿐만 아니라 전-방향 주행 기능이 요구되는 안내로봇, 탑승형 로봇, 이동수단 등에 필수적인 기술이 될 것이고 지능형서비스로봇 시장과 미래형 자동차시장의 확대에 기여할 수 있을 것이다.

• 한국식품과학회지
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• 제25권6호
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• pp.769-774
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• 1993

Fluidized bed opposed jet mill을 사용하여 초미세분쇄한 후 Turboplex classifier로 공기분급한 탈지미강분말의 입도는 air classifying wheel speed (ACWS)가 낮아짐에 따라 입자의 크기와 표준편차는 증가하고 단위부피당 표면적은 감소하였다. ACWS 21,000rpm에서 분급한 미강분말의 형태는 구형이었으며 입도 median이 $3.7{\mu}m$이었다. ACWS별로 회수된 시료의 단백질, 지방, 회분은 ACWS에 따라 전반적으로 증가하는 경향이었다. Mg, Zn, Fe 및 Mn 함량은 ACWS가 증가할수록 비교적 증가하는 경향을 보였으며, phytic acid함량은 중간 ACWS에서 약간 높은 값을 보였다. 식이섬유함량은 $25.2{\sim}31.5%$의 값을 보였고, ACWS 15,000rpm에서 최대값을 나타내었다. ACWS에 따른 시료의 색도는 ACWS가 높을수록 백색도(L)가 증가하였고, 적색도(a)와 황색도(B)는 감소하는 경향을 나타내었다. 보수력(WHC)은 12,000rpm에서 2.88g/g solid로 가장 높았고 ACWS가 높아짐에 따라 감소하는 추세를 보였으나, 보유력은 반대로 ACWS에 따라 약간 증가하는 경향을 보였다. 분급된 미강분말 현탁액의 유동특성은 Bingham body에 속하였으며 농도와 ACWS가 증가함에 따라 항복응력 및 점도가 상승하였다. 분급된 미강분말을 5% 수준으로 대체하여 케이크를 제조한 경우 대조구보다 케이크의 높이와 부피가 증가하였다.

• 한국기계가공학회지
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• 제13권1호
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• pp.92-99
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• 2014

An aspherical lens, which resolves several problems with a spherical lens,typically serves asa key part of an optical system. Generally, an aspherical lens is fabricated using a diamond turning machine or by mean of injection molding. However, residual stress and/or tool marks can arise when using a commercial fabricating method such as DTM or injection molding. A polishing process, thus, is commonly used to obtain a high-precision aspherical lens. In this study, a polishing method using MR fluid was applied to minimize several problems, in this case residual stress and the creation of tool marks, during the cutting process. The MR polishing system was developed to polish aspherical lenses. A series of experiments were performed to obtain a very fine surface roughness. PMMA (the lens material for molding) was used as a workpiece, and the gap size, magnetic field intensity, wheel speed and feed rate were selected as the parameters in this study. Finally, a very fine surface roughness of Ra=2.12nm was obtained after MR polishing.

• 천문학논총
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• 제20권1호
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• pp.143-149
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• 2005

KASI (Korea Astronomy and Space Science Institute) is developing the near-infrared camera system named KASINICS (KASI Near-Infrared Camera System) which will be installed at the 60cm f/13.5 Ritchey-Chretien telescope of the Sobaeksan Optical Astronomy Observatory (SOAO). The camera system is optimized for JHKL bands and has a 6 arcmin FOV. The optical system consists of two spherical mirrors and a 8-position filter wheel. With the exception for the dewar window, all optical elements are cooled inside cryogenic dewar. Since the Offner system is adopted to prevent thermal noises from outside of the telescope primary mirror, the secondary mirror of the Offner system acts as a cold Lyot stop. The optical performance does not change by temperature variations because the Aluminum mirrors contract and expand homogeneously with its mount. We finished the design and fabrication of the optical parts and are now aligning the optical system. We plan to have a test observation on 2006 January.

• 천문학회보
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• 제35권1호
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• pp.36.2-36.2
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• 2010

The CQUEAN (Camera for QUasars in EArly uNiverse) is an optical CCD camera optimized for observation of high redshift objects. It is going to be attached to the cassegrain focus of 2.1m telescope at McDonald Observatory, USA. We are making a focal reducer for CQUEAN to secure a larger field of view. The focal reducer is composed of four spherical lens, and it reduces the focal length of telescope by one third. We designed the lens configuration, performed tolerance analysis, and estimated the optical performance with ZEMAX. The differences in optical performace with/without filters were also investigated. The result from ZEMAX shows that the system has ample margin of errors for median seeing of 1.2" at McDonald observatory. Even with aberration and alignment tolerance, the performance is better than the original requirement. The lenses are now being made, and the lens barrel and an adapter for assembly of the Andor CCD camera and the filter wheel is now under designing process. We expect that the manufacturing of the focal reducer system as well as its optical test will be finished by April 2010.

• Design & Manufacturing
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• 제2권1호
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• pp.33-38
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• 2008

As consumer in optics, electronics, aerospace and electronics industry grow, the demand for ultra precision aspherical surface lens increases higher. Precision turning with single-diamond tools has a long history of development for fabrication of optical quality surfaces since the advent of aerostatic rotary spindles and precise linear motion guide ways. To enhance the precision and productivity of ultra precision aspherical surface micro lens, the following specification of ultra precision grinding system is required: the highest rotational speed of the grinder is 100,000rpm and its turning accuracy is $0.1{\mu}m$, positioning accuracy is $0.1{\mu}m$. The development process of the grinding system for the ultra precision aspherical surface micro lens for optoelectronics industry is introduced. In the work reported in this paper, an intelligent grinding system for ultra precision aspherical surface machining was designed by considering the factors affecting the surface roughness and profiles accuracy. An aerostatic form was adopted to build the spindle of the workpiece and the spindle of grinder and ultra precision LM guide way was adopted in this system. And this paper deals with mirror grinding of an aspheric surface micro lens by resin bonded diamond wheel and spherical lens of BK7. It results was that a form accuracy of $0.6{\mu}m$ P-V and a surface roughness of $0.006{\mu}m$ Rmax.

• 천문학논총
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• 제36권3호
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• pp.79-95
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• 2021

This study aims to develop a restoration model of an armillary sphere of Tongcheon-ui (Pan-celestial Armillary Sphere) by referring to the records of Damheonseo (Hong Dae-Yong Anthology) and the artifact of an armillary sphere in the Korean Christian Museum of Soongsil University. Between 1760 and 1762, Hong, Dae-Yong (1731-1783) built Tongcheon-ui, with Na, Kyung-Jeok (1690-1762) designing the basic structure and Ann, Cheo-In (1710-1787) completing the assembly. The model in this study is a spherical body with a diameter of 510 mm. Tongcheon-ui operates the armillary sphere by transmitting the rotational power from the lantern clock. The armillary sphere is constructed in the fashion of a two-layer sphere: the outer one is Yukhab-ui that is fixed; and the inner one, Samsin-ui, is rotated around the polar axis. In the equatorial ring possessed by Samsin-ui, an ecliptic ring and a lunar-path ring are successively fixed and are tilted by 23.5° and 28.5° over the equatorial ring, respectively. A solar miniature attached to a 365-toothed inner gear on the ecliptic ring reproduces the annual motion of the Sun. A lunar miniature installed on a 114-toothed inner gear of the lunar-path ring can also replay the moon's orbital motion and phase change. By the set of 'a ratchet gear, a shaft and a spur gear' installed in the solstice-colure double-ring, the inner gears in the ecliptic ring and lunar-path ring can be rotated in the opposite direction to the rotation of Samsin-ui and then the solar and lunar miniatures can simulate their revolution over the period of a year and a month, respectively. In order to indicate the change of the moon phases, 27 pins were arranged in a uniform circle around the lunar-path ring, and the 29-toothed wheel is fixed under the solar miniature. At the center of the armillary sphere, an earth plate representing a world map is fixed horizontally. Tongcheon-ui is the armillary sphere clock developed by Confucian scholars in the late Joseon Dynasty, and the technical level at which astronomical clocks could be produced at the time is of a high standard.