• 한국광학회:학술대회논문집
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• 한국광학회 2000년도 하계학술발표회
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• pp.3-3
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• 2000

Adaptive Optical (AO) technology can compensate for wave-front errors in real-time to improve image and beam quality. The research and development on AO in China began in 1979. In 1980, the first laboratory on AO in China was established in Institute of Optics and Electronics (IOE), Chinese Academy of Sciences (CAS). Since then several AO systems have been built in this Laboratory. The 19-element system is the first AO system in the world ever used in inertial confinement fusion (ICF) facility in our knowledge. It corrects the static error of this large laser engineering. The 21-element system was firstly tested at the 1.2m telescope of Kunming Observatory in 1990 and then up-dated as an IR AO system installed at the 2.16m telescope of Beijing Observatory. The 37-element system was used with a turbulence cell in Laboratory on Atmospheric Optics in Hefei to conduct elementary research on Atmospheric Optics. The 61-element system for astronomical observation is newly developed. It has been successfully installed at the 1.2m telescope of Kunming Observatory and a laser guide star system will be integrated with the system. A compact AO system using our newly developed miniature DM for high resolution ophthalmic imaging of retina is also being built. The key elements of these AO systems, deformable mirrors and fast-steering mirrors, are all developed in this Laboratory. In this talk, the main configurations of these AO systems, some test results as well as the specifications of these active mirrors will be presented.

• Current Optics and Photonics
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• 제5권2호
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• pp.101-113
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• 2021

Adaptive optics (AO) systems are becoming more complex to improve their optical performance and enlarge their field of view, so it is a hard and time consuming process to set up and optimize the components of AO systems with actual implementation. However, simulations allow AO scientists and engineers to experiment with different optical layouts and components without needing to obtain and prepare them physically. In this paper, we introduce a new AO simulation named the Korea Adaptive Optics Simulation (KAOS), independently developed by LIG Nex1. We verified the performance of KAOS by comparing with other AO simulation tools. In the comparison simulation, we confirmed the results from KAOS and other AO simulation tools were very similar. Also, we proposed a laser tomography AO system with five Rayleigh laser guide stars (LGSs) optimized by using KAOS to overcome the disadvantages of the AO system with a single sodium LGS for the satellite imaging system. We verified the performance of the proposed AO system using KAOS, and the simulation result showed averaged Strehl ratio of 0.37.

• 대한환경공학회지
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• 제30권6호
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• pp.666-672
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• 2008

수산물 가공폐수를 AO$_2$공법에 적용하여 유기물, 질소, 인의 동시제거 가능성을 평가 하였다. 처리도 실험은 도시하수처리장에서 가져온 활성슬러지를 담체에 2주 이상 부착시킨 후 반응조 부피 25%로 충진하여 실험을 행하였다. 유입수 농도는 실험기간 동안 COD : 198 - 1,240 mg/L, TN : 75 - 577.4 mg/L, TP : 2.2 - 53.5 mg/L였다. 운전기간동안 평균 제거효율은 COD : 86.5%(65.7 mg/L), TN : 81.4%(53.1 mg/L), TP : 80.6%(4.07 mg/L)로 나타났다. Anaerobic조와 Aerobic조로 구성된 시스템에 유기물 및 영양염류 부하율이 증가되어도 비교적 안정된 형태의 운전이 가능하였다. 사용된 PU-AC 메디아는 높은 MLSS량을 보유하여 AO$_2$ 시스템 내에서 생물학적 처리율을 높일 수 있었던 것으로 사료된다.

• International journal of advanced smart convergence
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• 제6권2호
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• pp.51-58
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• 2017

Recently, rapid advances of Ethernet and IP technology have brought many changes in the sound industry. In addition, due to AoIP-based audio transmission technology, various problems of the acoustic system (sound quality deterioration due to long distance transmission, complicated wiring) have improved dramatically. However, when many distributed audio systems are connected with AoIP equipment, if there is a problem in the equipment, it is impossible to operate the connected system. AoIP equipment only can transmit audio signals but cannot adjust the system for acoustic environment. In this paper, AoIP equipment is to be installed with sound equipment on a one-to-one basis, so that various existing problems can be solved and adjustment of sound quality (reverberation, echo, delay and EQ) can be possible by AoIP-based OAC (On-site Audio Center) with built-in DSP function. As a result, uncompressed real-time transmission by distributed transmission/receipt module in OAC (On-site Audio Center) and high quality sound by adjustment of sound quality with built-in DSP can be acquired. It is expected that OAC based sound system will be the industry standard in ubiquitous environment.

• 천문학회보
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• 제46권2호
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• pp.53.3-53.3
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• 2021

Adaptive Optics (AO) was first studied in the field of astronomy, and its applications have been extended to the field of laser, microscopy, bio, medical, and free space laser communication. AO modelling and simulation are required throughout the system development process. It is necessary not only for proper design but also for performance verification after the final system is built. In KASI, we are trying to develop the AO Python Package for AO modelling and simulation. It includes modelling classes of atmosphere, telescope, Shack-Hartmann wavefront sensor, deformable mirror, which are the components for an AO system. It also includes the ability to simulate the entire AO system over time. It is being developed in the Super Eye Bridge project to develop a segmented mirror, an adaptive optics, and an emersion grating spectrograph, which are future telescope technologies. And it is planned to be used as a performance analysis system for several telescope projects in Korea.

• International journal of advanced smart convergence
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• 제6권2호
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• pp.1-8
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• 2017

Recently, the development of the information communication industry has made many changes in the industrial acoustic industry. Especially, it has a great influence on the change of system and equipment of acoustic system. Analog equipment is changing to digital equipment, and integrated control equipment makes it easier to operate and manage the sound system. However, the integrated control system currently on the market is only controllable for some devices. In this paper, we propose a new AoIP - based system configuration method, which enables the operation status monitoring, unmanned operation and self - diagnosis of equipment. As a result of the study, it is confirmed that the proposed system can be operated, monitored, and self - diagnosed at remote sites. It is expected that an AoIP- based sound system will be the industry standard in the future.

• Current Optics and Photonics
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• 제8권2호
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• pp.183-191
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• 2024

High-resolution retinal imaging based on adaptive optics (AO) is important for early diagnosis related to retinal diseases. However, in practical applications, closed-loop AO correction takes a relatively long time, and traditional open-loop correction methods have low accuracy in correction, leading to unsatisfactory imaging results. In this paper, a SH-U-net-based open-loop AO wavefront correction method is presented for a retinal AO imaging system. The SH-U-net builds a mathematical model of the entire AO system through data training, and the Root mean square (RMS) of the distorted wavefront is 0.08λ after correction in the simulation. Furthermore, it has been validated in experiments. The method improves the accuracy of wavefront correction and shortens the correction time.

• 공업화학
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• 제7권1호
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• pp.83-90
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• 1996

AO-AOT계내에서 S/D의 증가에 따라 흡수 및 형광 spectra의 변화 양상이 감소하다가 증가함을 알 수 있으며 회합 및 해리가 일어남을 알 수 있다. 그리고 온도 상승에 따라 순수한 AO계에서는 흡광도가 증가하나 premicellar영역(S/D=10, 20, 50 및 80)내에서는 흡광도가 오히려 점차 감소한다. 한편 AO-AOT계에 첨가한 염의 농도가 증가함에 따라 metachromasy 소멸도는 증가하나 $NaNO_3$의 경우는 이와 반대로 나타난다. 이러한 염의 양이온에 대한 metachromasy 소멸도의 증가 순서는 $Li^+$, $Na^+$ > $Mg^{2+}$ > $Ca^{2+}$이며, 염의 음이온에 대해서는 $Cl^-$ > $SO_4{^{2-}}$ > $NO_3{^-}$로 나타남을 알 수 있었다.

• 천문학회보
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• 제45권1호
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• pp.67.1-67.1
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• 2020

Adaptive Optics (AO) is the technology for ground-based telescopes to overcome the interference caused by atmospheric turbulence. We are developing an AO system for the 1-m telescope at Seoul National University Observatory (SNUO). The seeing size of the SNUO is 2 arcseconds on average, and 0.85 arcseconds at best condition. Our system is based on MEMS deformable mirror and Shack-Hartmann wavefront sensor. We developed the wavefront sensor using a cheap CMOS camera, and measured phase disturbance at SNUO. To verify the performance of the AO system, we designed an artificial phase disturber that produces similar scale phase error, measured at SNUO. We carried out laboratory tests in which the AO system measures and corrects the wavefront using the phase disturber and an F/6 light source, the same as that of SNUO telescope. The control system was developed in C++. The system performs closed-loop PI correction up to 100 Hz at a consumer-grade PC.

• Journal of Astronomy and Space Sciences
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• 제9권1호
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• pp.41-51
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• 1992

근접쌍성 AO Can과 AW Cam을 1984년의 관측 계절에 소백산 천문대의 61cm 반사 망원경으로 광전 관측하였다. 이 두별의 관측으로 부터 AO Cam의 채 1 극심시각 l개와 AW Cam익 체 1 극심시각 3 개를 각각 구하였다. 여러 문헌으로 부터 수집한 이 두 별의 극심시각들을 이용하여 최소자송법으로 A0 Cam파 AW Cam의 새로운 광도요소를 구하였다. AO Cam의 공전주기는 1980년 10월(JD 2444520) 부터 1985년 2월 (JD 2446107)까지 일정하였다. 그러나 최근에 Mullis와 Faulkner (1991)가 발표한 AO Cam의 l개의 제2극심시각 (JD 2447864. 7879)은 우리가 새로 구한 광도요소와 약 +4.6분 ( (0.0032일)의 큰 차이가 난다. AO Carn의 극심시각의 앞으로의 관측은 이 별의 공전주기 변화 연구에 중요하다. AW Cam의 공전주기는 지난 1930년대 초 이래 현재짜지 약 60년 동안 P=$0^d.77134645$로 일정하다