• Journal of Information Display
• /
• 제3권3호
• /
• pp.30-34
• /
• 2002

CRTs can be improved by means of magnetic quadrupoles. Areas of improvement are convergence, spot shape, image-flatness and space charge compensation.

• 한국정밀공학회:학술대회논문집
• /
• 한국정밀공학회 2010년도 추계학술대회 논문집
• /
• pp.607-608
• /
• 2010

• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2009년도 제36회 동계학술대회 초록집
• /
• pp.132.2-132.2
• /
• 2009

• Journal of the Optical Society of Korea
• /
• 제19권3호
• /
• pp.237-240
• /
• 2015

We derived the average bit error rate (BER) of coherent free-space optical (FSO) systems with digital binary phase shift keying (BPSK) modulations over atmospheric turbulence channels with a gamma-gamma distribution. To obtain a generalized derivation in a closed-form expression, we used special integrals and transformations of the Meijer G function. Furthermore, we numerically analyzed and simulated the average BER behavior according to the average SNR for different turbulence strengths. Simulation results are demonstrated to confirm the analytical results.

• Smart Structures and Systems
• /
• 제21권6호
• /
• pp.777-791
• /
• 2018

This paper discusses the shape control of deformable mirrors for Adaptive Optics in the dynamic range. The phenomenon of control-structure interaction appears when the mirror becomes large, lowering the natural frequencies $f_i$, and the control bandwidth $f_c$ increases to improve the performance, so that the condition $f_c{\ll}f_i$ is no longer satisfied. In this case, the control system tends to amplify the response of the flexible modes and the system may become unstable. The main parameters controlling the phenomenon are the frequency ratio $f_c/f_i$ and the structural damping ${\zeta}$. Robustness tests are developed which allow to evaluate a lower bound of the stability margin. Various passive and active strategies for damping augmentation are proposed and tested in simulation.

• 한국광학회지
• /
• 제8권5호
• /
• pp.431-437
• /
• 1997

광신호 상호연결 및 입력물체의 결상을 위한 기존의 평판광학계에서는 굴절률이 일정한 유리기판을 광신호 전달매체로 사용하였는데 반하여, 본 연구에서는 물매-굴절률(gradient-index) 분포를 갖는 기판을 사용하는 새로운 개념의 평판광학계를 제안하였다. 물매기판에 의한 결상특성을 근축광선 추적에 의해 분석하였으며, 입력 광신호의 위치에 따라 결상된 위치가 변하는 실험결과로부터 새로운 결상광학계로의 응용 가능성을 검증하였다. 그리고, 물매기판을 이용한 평판광학계가 하나의 입력신호를 여러 출력면으로 동시에 분배할 수 있는 광신호처리계로도 응용될 수 있음을 제시하였다.

• 천문학회보
• /
• 제46권2호
• /
• pp.75.2-76
• /
• 2021

MESSIER is a science satellite project to observe the Low Surface Brightness (LSB) sky at UV and optical wavelengths. The wide-field, optical system of MESSIER is optimized minimizing optical aberrations through the use of a Linear Astigmatism Free - Three Mirror System (LAF-TMS) combined with freeform mirrors. One of the key factors in observations of the LSB is the shape and spatial variability of the Point Spread Function (PSF) produced by scatterings and diffraction effects within the optical system and beyond (baffle). To assess the various factors affecting the PSF in this design, we use PhoSim, the Photon simulator, which is a fast photon Monte Carlo code designed to include all these effects, and also atmospheric effects (for ground-based telescopes) and phenomena occurring inside of the sensor. PhoSim provides very realistic simulations results and is suitable for simulations of very weak signals. Before the application to the MESSIER optics system, PhoSim had not been validated for confocal off-axis reflective optics (LAF-TMS). As a verification study for the LAF-TMS design, we apply Phosim sequentially. First, we use a single parabolic mirror system and compare the PSF results of the central field with the results from Zemax, CODE V, and the theoretical Airy pattern. We then test a confocal off-axis Cassegrain system and check PhoSim through cross-validation with CODE V. At the same time, we describe the shapes of the freeform mirrors with XY and Zernike polynomials. Finally, we will analyze the LAF-TMS design for the MESSIER optical system.

• 한국안광학회지
• /
• 제7권2호
• /
• pp.197-202
• /
• 2002

본 논문에서는 telecentric 렌즈에 대하여 간략하게 그 성질을 알아보고 기존에 설계된 profile projection lens를 선택하여 광학적 성능을 조사하여 봄으로서 telecentric에 관한 이해를 도모하고자 하였다. 분석한 광학계는 F-no가 2.8이고, 첫 번째 렌즈를-렌즈로 사용하여 물측 초점의 위치를 광학계 안쪽에 위치시킴으로서 aperture stop을 광학계 내부에 설치하게 하여 광학계를 보다 compact하게 하려 하였음을 알 수가 있었다. 시야는 $21^{\circ}$ 정도를 유지하며, entrance pupil이 물측 초점의 위치(FFL)에 놓여짐으로써 exit pupil은 -49404.1mm로 물측 공간쪽으로 무한대로 놓여지게 됨을 확인할 수가 있다. 이로서 본 광학계는 '상측이 텔레센트릭계(image space telecentricity)'의 한 형태라고 할 수 있다.

• 천문학회지
• /
• 제46권4호
• /
• pp.161-172
• /
• 2013

A focal reducer is developed for CQUEAN (Camera for QUasars in EArly uNiverse), which is a CCD imaging system on the 2.1 m Otto Struve telescope at the McDonald observatory. It allows CQUEAN to secure a wider field of view by reducing the effective focal length by a factor of three. The optical point spread function without seeing effects is designed to be within one pixel ($0.283^{\prime\prime}$) over the field of view of $4.82^{\prime}{\times}4.82^{\prime}$ in optimum wavelength ranges of 0.8-1.1 ${\mu}m$. In this paper, we describe and discuss the characteristics of optical design, the lens and barrel fabrications and the alignment processes. The observation results show that the image quality of the focal reducer confirms the expectations from the design.

• 천문학회보
• /
• 제37권1호
• /
• pp.76.2-76.2
• /
• 2012

The understanding spectral characterization of possible earth-like extra solar planets has generated wide interested in astronomy and space science. The technical central issue in observation of exoplanet is deconvolution of the temporally and disk-averaged spectra of the exoplanets. The earth model based on atmospheric radiative transfer method has been studied in recent years for solutions of characterization of earthlike exoplanet. In this study, we report on the current progress of the new method of 3D earth model as a habitable exoplanet. The computational model has 3 components 1) the sun model, 2) an integrated earth BRDF (Bi-directional Reflectance Distribution Function) model (Atmosphere, Land and Ocean) and 3) instrument model combined in ray tracing computation. The ray characteristics such as radiative power and direction are altered as they experience reflection, refraction, transmission, absorption and scattering from encountering with each all of optical surfaces. The Land BRDF characteristics are defined by the semi-empirical "parametric-kernel-method" from POLDER missions from CNES. The ocean BRDF is defined for sea-ice cap structure and for the sea water optical model, considering sun-glint scattering. The input cloud-free atmosphere model consists of 1 layers with vertical profiles of absorption and aerosol scattering combined Rayleigh scattering and its input characteristics using the NEWS product in NASA data and spectral SMARTS from NREL and 6SV from Vermote E. The trial simulation runs result in phase dependent disk-averaged spectra and light-curves of a virtual exoplanet using 3D earth model.