• 전자공학회논문지A
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• 제31A권12호
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• pp.135-141
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• 1994

A linear BiCMOS operational transconductance amplifier (OTA) is described. It consists of a CMOS linear transconductor and a bipolar translineear current gain cell followed by three CMOS current mirrors. The proposed circuit has comparable linearity and temperature stability but superior dc characteristics to its bipolar counterpart. A test circuit with a transconductance of 47.3$\mu$s has been simulated. Simulation results show that a linearity error of less than $\pm$1 percent over an input volgate range from -1.0 to 1.0 V and a output dc offset current as small as-3.6 nA can be obtained.

• 천문학회지
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• 제29권spc1호
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• pp.279-280
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• 1996

This paper reports on the outline and the status of the TAMA-300 project, the 300 meter laser interferometer gravitational wave detector developed by a team of scientists of several research institutes and universities in Japan. In fact the project has been funded and its construction started at the National Astronomical Observatory, Mitaka, in spring 1995. And the constructions of the tunnels for the east-west and north-south arms and of the central building are completed and a half of pipes for laser beams were brought in. Very stable laser oscillator has been almost completed and mew techniques such as vibration isolations, recycling of laser power, and suspension of mirrors by double pendulums have been developed. In fact the purposes of the project are to establish techniques necessary for future km-class detectors and to operate the detector to catch possible gravitational wave events in nearby galaxies such as Andromeda, the target sensitivity being $3 {\times} 10^{-21}$ at 300Hz.

• 천문학회보
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• 제42권2호
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• pp.54.2-54.2
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• 2017

While quasars are sparse in number density, they reside at relatively high-redshift as compared to e.g. luminous red galaxies. Hence, they are likely to be less non-linearly evolved than the galaxy population, and thus have a distribution that more closely mirrors the primordial density field. Therefore, they offer an intriguing opportunity to search for Baryonic Acoustic Oscillations (BAO). To this end, the 3-point correlation function (3PCF) is an excellent statistical tool to detect BAO. In this work, we will make the first-ever measurement of the large-scale quasar 3PCF from the SDSS-IV DR14 quasar sample (spanning the largest volume to-date). This work will use the order N2-time 3PCF algorithmof Slepian & Eisenstein (2015), with N the number of objects.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2003년도 춘계학술대회 논문집
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• pp.1881-1884
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• 2003

Diamond turning machines have, been used for the processing of surface like a mirror with the control scheme of minimizing shape error, Ultra-precision diamond fuming is applied to produce highly precision optical components required not only a high machining accuracy but also a good surface roughness. Al-6061 is widely used as optical parts such as laser reflector's mirror or multimedia instrument. In this study, thermal-imaged Al flat mirrors are fabricated by SPDT. The surface roughness 3.472 nm Ra, power 2 fringe(at 632.8 nm) and irregularity 1 fringe(at 632.8 nm) for form waviness of thermal-imaged Al flat mirror are very satisfied to the required specification in industry.

• 대한인간공학회지
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• 제29권2호
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• pp.249-255
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• 2010

The visibility evaluation is significant for the development of construction equipment. The visibility evaluation follows the standards of ISO 5006, ISO 14401-1, and ISO 14401-2. The evaluation contains the operator's visibility and the visibility of rear-view mirrors. The operator's visibility includes the visibility test which requires the recognition of the rectangular line surrounding the machine by one meter and the circle with a 12 meter radius. This study describes the two evaluation processes for the development of the wheel loader. The first process is the light bulb shadow test by using a prototype wheel loader. The second process is based on computer simulation in virtual space. The advantages and disadvantages of computer simulation process are investigated.

• 한국광학회:학술대회논문집
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• 한국광학회 2004년도 하계학술발표회
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• pp.64-67
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• 2004

The optics and opto-mechanics are disigned for imaging the sun at Lyman-${\alpha}$ line for scientific satellite. The optics are composed of conic mirrors. In order to block stary light. the new baffle design method is suggested. And we will present the opto-mechanics for this scientific satellite.

• 한국광학회지
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• 제5권1호
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• pp.60-66
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• 1994

양영역 불안정형(Positive Branch Unstable) Nd:YAG 레이저 공진기를 모델링하여 공진기내의 TE$M_{00}$ 기본모우드의 waist에 대한 수치해석을 하였으며 이를 토대로 레이저 공진기를 설계 제작하였다. 레이저봉의 열렌즈 초점거리를 측정하였으며 이를 이용하여 빔 waist에서의 TE$M_{00}$ 모우드의 spot size에 대한 계산치와 실험치를 비교하였다. 그리고 고반복률로 발진하는 다중모우드(multimode)의 spot size를 측정하여 beam quality factor $M^2$을 산출하였다. 한편 불안정 공진기에서 얻어진 출력실험 결과를 Plane-Parallel 공진기의 경우에 비교하여 그 특성을 평가하였다.

• 한국광학회지
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• 제5권2호
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• pp.212-216
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• 1994

원적외선 영역인 $8-12.\mu$m 대역의 열상장비 주사광학계를 설계 제작하였다. 검출기로 5개 소자의 SP-RITE HgCdTe를 사용하는 직병렬 주사를 위해 수평 및 수직주사에는 각각 회전다면거울과 진동평면거울을 사용하였으며, 주사연결거울로는 구면거울을 사용하여 주사거울의 크기 및 입사동에서의 동수차를 최소화 하였다. 주사광학계는 $40^{\circ}\times26.67^{\circ}$의 넓은 주사시야를 갖는다. 회절 변조전달함수의 계산결과 회절한계의 성능을 만족하였으며 제작 및 시험 결과 고분해능의 열영상을 얻을 수 있었다.

• 한국광학회:학술대회논문집
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• 한국광학회 2000년도 제11회 정기총회 및 00년 동계학술발표회 논문집
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• pp.124-125
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• 2000

We introduce a scheme with a maximized efficiency of detecting atoms passing through an optical standing-wave mode cavity. Consider a standing-wave optical cavity illuminated by a weak probe beam through one of its mirrors where the transmission through the other mirror is monitored by a photodetector. If an atom is put in the cavity, the atom-cavity coupling shifts the resonance frequency of the system via the so-called normal mode splitting, and thereby the transmission power will drop. In fact, this type of atom detection scheme has been used in recent single atom trap experiments In practice, however, the field in a standing-wave mode will have a geometrical structure having nodes and antinodes that when the atom traverses the cavity through one of the nodes, there will be no such effect of atom-field interaction. (omitted)

• Journal of the Optical Society of Korea
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• 제13권2호
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• pp.184-192
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• 2009

There are total eight degrees of freedom in designing a three-mirror system. If we correct four kinds of third order aberrations and the system should have the specified effective focal length, the remaining three degrees of freedom can be used for selecting a suitable configuration for a specific application. We suggest an analytic design procedure for a three-mirror telescope system which has a suitably sized secondary mirror and proper separations between mirrors, and is corrected for four kinds of third order aberrations, spherical aberration, coma, astigmatism, and field curvature. Two design examples are shown. One has a compact configuration with off-axial field, the other has relatively long configuration with annular ring field.