• 한국위성정보통신학회논문지
• /
• 제1권1호
• /
• pp.26-39
• /
• 2006

영상 레이다(SAR)는 전천후 영상획득이 가능하며, 반사표면의 물리적인 구조와 특성에 따라 표적탐지 및 식별성능이 우수하므로 군사용으로는 물론 과학 민수용으로 광범위한 활용분야를 가지고 있다. 본 논문에서는 먼저 X-밴드 소형위성 SAR 체계 설계 개념과 주요 임무 및 체계설계 요건들을 제시하고 이를 만족시키기 위한 영상모드 설계 기법과 표준 영상모드 설계 결과를 분석한다. 그리고, X-밴드 SAR 탑재체 및 지상 수신처리의 주요 체계 설계 결과와 성능특징을 제시하고, 마지막으로 SAR 영상활용을 위한 응용분야와 처리결과를 제시한다. 제안된 위성 SAR 시스템은 광역감시 모드에서 고해상도 모드까지 다양한 영상 모드 구현이 가능하며, 소형, 고성능, 저 비용 관점에서 효율적인 전천후 레이다 영상획득 시스템이다.

• 정보저장시스템학회논문집
• /
• 제2권1호
• /
• pp.79-84
• /
• 2006

The next generation of optical storage systems requires higher numerical aperture(NA) objective lenses and shorter wavelength laser in order to improve the unit areal density. A blu-ray technology satisfies a miniaturization and a high capacity which are the requirements of the portable device. In this paper, we analyze the optical performance of hybrid micro lens and do active alignment. The hybrid micro lens is manufactured by using a wafer based fabrication technology. Optical components of hybrid micro lens are evaluated. The measurement of the optical power, the spot size and the wavefront error are performed to evaluate the hybrid micro lens with NA 0.85. Using the measured data, we estimate if the performance of hybrid micro lens corresponds to the designed performance. After the performance of hybrid micro lens is evaluated. the integrated optical pickup and the hybrid micro lens are assembled by active alignment using UV curing and the optical performance of SFFOP is satisfied with BD specifications.

• 천문학회보
• /
• 제43권2호
• /
• pp.57.2-57.2
• /
• 2018

In astronomical observation, sequential device control and real-time data processing are important to maximize observing efficiency. We have developed series of automatic observing software (KAOS, KHU Automatic Observing Software), e.g. KAOS30 for the 30 inch telescope in the McDonald Observatory and KAOS76 for the 76 cm telescope in the KHAO. The series consist of four packages: the DAP (Data Acquisition Package) for CCD Camera control, the TCP (Telescope Control Package) for telescope control, the AFP (Auto Focus Package) for focusing, and the SMP (Script Mode Package) for automation of sequences. In this poster, we introduce KAOS10 which is being developed for controlling a small telescope such as aperture size of 10 cm. The hardware components are the QHY8pro CCD, the QHY5-II CMOS, the iOptron CEM 25 mount, and the Stellarvue SV102ED telescope. The devices are controlled on ASCOM Platform. In addition to the previous packages (DAP, SMP, TCP), KAOS10 has QLP (Quick Look Package) and astrometry function in the TCP. QHY8pro CCD has RGB Bayer matrix and the QLP transforms RGB images into BVR images in real-time. The TCP includes astrometry function which adjusts the telescope position by comparing the image with a star catalog. In the future, We expect KAOS10 be used on the research of transient objects such as a variable star.

• 한국멀티미디어학회논문지
• /
• 제25권7호
• /
• pp.895-902
• /
• 2022

Building segmentation using satellite imagery such as EO (Electro-Optical) and SAR (Synthetic-Aperture Radar) images are widely used due to their various uses. EO images have the advantage of having color information, and they are noise-free. In contrast, SAR images can identify the physical characteristics and geometrical information that the EO image cannot capture. This paper proposes a learning framework for efficient building segmentation that consists of a teacher-student-based privileged knowledge distillation and deformable convolution block. The teacher network utilizes EO and SAR images simultaneously to produce richer features and provide them to the student network, while the student network only uses EO images. To do this, we present objective functions that consist of Kullback-Leibler divergence loss and knowledge distillation loss. Furthermore, we introduce deformable convolution to avoid pixel-level noise and efficiently capture hard samples such as small and thin buildings at the global level. Experimental result shows that our method outperforms other methods and efficiently captures complex samples such as a small or narrow building. Moreover, Since our method can be applied to various methods.

• International Journal of Computer Science & Network Security
• /
• 제23권1호
• /
• pp.1-10
• /
• 2023

Open surface water body extraction is gaining popularity in recent years due to its versatile applications. Multiple techniques are used for water detection based on applications. Different applications of Radar as LADAR, Ground-penetrating, synthetic aperture, and sounding radars are used to detect water. Shortwave infrared, thermal, optical, and multi-spectral sensors are widely used to detect water bodies. A stereo camera is another way to detect water and different methods are applied to the images of stereo cameras such as deep learning, machine learning, polarization, color variations, and descriptors are used to segment water and no water areas. The Satellite is also used at a high level to get water imagery and the captured imagery is processed using various methods such as features extraction, thresholding, entropy-based, and machine learning to find water on the surface. In this paper, we have summarized all the available methods to detect water areas. The main focus of this survey is on water detection especially in small patches or in small areas. The second aim of this survey is to detect water hazards for unmanned vehicles and off-sure navigation.

• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2012년도 제43회 하계 정기 학술대회 초록집
• /
• pp.319-320
• /
• 2012

Large aperture optical modulator called optical shutter is a key component to realize time-of-flight (TOF) based three dimensional (3D) imaging systems [1-2]. The transmission type electro-absorption modulator (EAM) is a prime candidate for 3D imaging systems due to its advantages such as small size, high modulation performance [3], and ease of forming two dimensional (2D) array over large area [4]. In order to use the EAM for 3D imaging systems, it is crucial to remove GaAs substrate over large area so as to obtain high uniformity modulation performance at 850 nm. In this study, we propose and experimentally demonstrate techniques for backside etching of GaAs substrate over a large area having high uniformity. Various methods such as lapping and polishing, dry etching for anisotropic etching, and wet etching ([20%] C6H8O7 : H2O2 = 5:1) for high selectivity backside etching [5] are employed. A high transmittance of 80% over the large aperture area ($5{\times}5mm^2$) can be obtained with good uniformity through optimized backside etching method. These results reveal that the proposed methods for backside etching can etch the substrate over a large area with high uniformity, and the EAM fabricated by using backside etching method is an excellent candidate as optical shutter for 3D imaging systems.

• 대한전자공학회논문지
• /
• 제19권2호
• /
• pp.14-22
• /
• 1982

국내 최초로 대구경 카세그레인 안테나의 자체 설계및 제작기술을 연구하고 시작품에 대한 성능을 측정 비교하였다. 카세그레인 안테나의 설계에 있어서는 여러 문헌을 참고하여 그 설계 수순을 정하고 특히 선진국에서 인공위성으로 부터의 TV전파 직접수신용으로 지목하고 있는 직경 4.6m인 파라보라회사 반대 곡면형 카세그레인 안테나의 제작에 있어 파라보라 곡면의 12분의 1 크기의 소곡면의 정밀제작및 이들의 정밀조립에 힘썼고 주어진 복반사경에 대하여 일차복사기의 개구 크기와 위치가 최소차폐를 만족하도록 전산 설계하는데 주력하였다. 시작된 안테나의 제성능은 이득이 43dB, 최대 정재파비 1.15, 판치각 1.1°등으로 나타났으며 같은 유형의 외국제품에 비하여 천색이 없었다.

• 한국전자파학회논문지
• /
• 제21권11호
• /
• pp.1285-1294
• /
• 2010

무인 차량의 야지 자율 주행을 위한 목적으로 수풀 뒤쪽에 가려져 있는 장애물을 탐지하고 회피하기 위해 수풀을 투과하여 차량의 전방을 고해상도로 영상화 할 수 있는 근거리 초광대역 영상 레이다를 설계한다. 광대역 특성에 적합하고 배열 구성이 용이한 소형 평판형 비발디 안테나를 설계하고 방사 패턴 및 정재파비를 측정한다. 영상의 거리 해상도를 기준으로 대역폭을 분석하고, 방위각 해상도를 기준으로 수신용 배열 안테나를 설계한다. 수신용 배열 안테나의 간격과 영상 해상도 및 표적의 신호 중첩 관계를 분석한다. 수풀로 부터 반사되는 신호를 수신하기 위해 회로망 분석기를 이용하여 계단 주파수 파형을 사용하는 합성 개구면 레이다를 구성한다. 제안한 방법은 수풀에서 코너 반사기를 위치시키고 이것의 반사 신호를 영상화함으로써 수풀의 투과 특성 및 레이다 영상의 해상도를 분석하여 무인 차량에 적용가능성을 보인다.

• Progress in Superconductivity
• /
• 제5권2호
• /
• pp.98-104
• /
• 2004

We analyzed a noise-sensitivity profile of a specific SQUID sensor system for the localization of brain activity. The location of a neuromagnetic current source is estimated from the recording of spatially distributed SQUID sensors. According to the specific arrangement of the sensors, each site in the source space has different sensitivity, that is, the difference in the lead field vectors. Conversely, channel noises on each sensor will give a different amount of the estimation error to each of the source sites. e.g., a distant source site from the sensor system has a small lead-field vector in magnitude and low sensitivity. However, when we solve the inverse problem from the recorded sensor data, we use the inverse of the lead-field vector that is rather large, which results in an overestimated noise power on the site. Especially, the spatial sensitivity profile of a gradiometer system measuring tangential fields is much more complex than a radial magnetometer system. This is one of the causes to make the solutions of inverse problems unstable on intervening of the sensor noise. In this study, in order to improve the localization accuracy, we calculated the noise-sensitivity profile of our 40-channel planar SQUID gradiometer system, and applied it as a normalization weight factor to the source localization using synthetic aperture magnetometry.

• 한국전자파학회논문지
• /
• 제20권11호
• /
• pp.1201-1208
• /
• 2009

도래각 추정 알고리즘의 분해능은 배열 안테나 개구면의 크기에 비례한다. 따라서 인접한 코히런트 신호를 개구면이 작은 배열 안테나를 이용하여 분해하는 것은 한계가 있다. 이러한 한계를 극복하기 위해 본 논문에서는 가상 확장 배열 안테나에 대한 공간 스펙트럼들의 특성을 이용하여 분해능을 향상시키는 방안을 제시하였다. SNR이 -10 dB에서 0 dB를 갖는 코히런트 신호가 원형 배열 안테나에 입사할 경우를 시뮬레이션한 결과, 표준 DML 알고리즘은 입사 신호를 전혀 분해할 수 없었으나, 제안한 DML 알고리즘은 100 % 분해 가능함을 확인하였다.