• 한국광학회지
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• 제33권3호
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• pp.99-105
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• 2022

자유 공간 광통신 시스템에서 발생하는 대기 외란에 의한 광신호 변동을 억제하기 위하여 전광(all-optical) 자동 이득 조절(automatic gain controlled, AGC) 어븀 첨가 광섬유 증폭기(erbium-doped fiber amplifier, EDFA)를 활용할 때의 성능을 실험적으로 평가하였다. EDFA에 입력되는 광신호 입력을 -30 dBm과 -10 dBm으로 각각 설정하여 증폭기가 소 신호 영역과 포화 영역에서 동작할 때의 성능을 실험적으로 비교하였다. 이 때 광신호의 요동은 음향 광학 변조기(acousto-optic modulator, AOM)를 활용하여 구현하였다. 실험 결과로부터 EDFA가 소 신호 영역에서 동작하며, 피드백되는 증폭된 자발 방출(amplified spontaneous emission, ASE) 광 전력이 0 dBm으로 증폭기를 포화시킬 수 있는 경우에 가장 작은 광신호 요동 특성을 얻을 수 있음을 확인하였다.

• 대한의생명과학회지
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• 제7권2호
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• pp.71-77
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• 2001

To evaluate the effect of occlusive skin on the activity of cutaneous oxygen free radical metabolizing enzymes in rats, the dorsal skin was covered with closed glass chamber shaped petri dish, 46 mm in diameter and 10 mm in height and sealed by an adhesive. Five day-occluded group showed more increased activity of xanthine oxidase (XO) than that of control, and the activity of five day-occluded group was higher than that of ten day-occluded group. The activities of superoxide dismutase (SOD) and glutathione peroxidase (GPx) were significantly higher in ten day-occluded group than in control or five day-occluded group. All the more, five day-occluded group showed the decreasing tendency of SOD and GPx activities compared to those of control. On the other hand, the cerrous perhydroxide deposits were observed in the intercellular space of the stratum basale in five day-occluded group under the electronic microscope using a cytochemistry method. Futhermore, the degree of cerrous perhydroxide reaction was lower in ten day-occluded group than in five day-occluded group. In conclusion, the increased XO activity and the decreased SOD and GPx activities are likely to responsible far the accumulation of $H_2O_2$ in five day-occluded group.

• 한국광학회지
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• 제19권3호
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• pp.242-245
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• 2008

본 논문에서는 $1{\times}4$ 스위치와 서로 다른 FSR(free spectral ranges)을 갖는 마이크로링 공진기 배열을 결합하여 구현된 광공진기 라우터를 기반으로 하는 집적광학 방식의 4채널 선택 마이크로웨이브(microwave: MW) 필터를 제안하고 구현하였다. 중심 주파수는 링 공진기의 반지름에 따른 FSR에 의해 결정되며, 이를 통해 얻어지는 10 GHz, 16 GHz, 18 GHz, 20 GHz로 구성된 4개의 채널은 광스위치에 제어 전압을 인가하여 개별적으로 선택할 수 있었다.

• 한국광학회지
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• 제3권1호
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• pp.43-49
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• 1992

Marx generator와 진공 다이오드, Bifilar helical wiggler, 인도자장 솔레노이드 등을 이용하여 마이크로파 영역의 자유전자 레이저를 설계 제작하였다. Bifilar helical wiggler의 자장분포를 분석하였고 공간전하의 수직성분 효ㅗ가를 고려하여 계산한 전자궤적 모의실험을 통하여 Wiggler자장이 전자빔 입사에 적합함을 확인하였다. Wiggler자장 300G, 인도자장 4.4kG, 전자빔 에너지 170keV일때 분산방정식에 의하여 계산된 출력 주파수는 약 11GHz였고 실험 결과 나타난 출력 주파수의 점위는 9.78GHz-11.7GHz로 추정되었다. 전자 속도의 축방향 퍼짐을 고려하여 이론적으로 이득을 계산하였다.

• Journal of the Optical Society of Korea
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• 제20권1호
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• pp.55-63
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• 2016

In this paper, a new asymmetric public key cryptography based on the modified RSA algorithm is proposed by using logic-based optical processing. The proposed asymmetric public key algorithm is realized into an optical schematic, where AND, OR and XOR logic operations are implemented by using free space digital optics architecture. Schematically, the proposed optical configuration has an advantage of generating the public keys simultaneously. Another advantage is that the suggested optical setup can also be used for message encryption and decryption by simply replacing data inputs of SLMs in the optical configuration. The last merit is that the optical configuration has a 2-D array data format which can increase the key length easily. This can provide longer 2-D key length resulting in a higher security cryptosystem than the conventional 1-D key length cryptosystem. Results of numerical simulation and differential cryptanalysis are presented to verify that the proposed method shows the effectiveness in the optical asymmetric cryptographic system.

• Current Optics and Photonics
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• 제1권4호
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• pp.271-277
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• 2017

Based on the extended Huygens-Fresnel principle, the analytical propagation formulae for spectrally partially coherent Gaussian Schell-model pulsed (SPGSMP) beams propagating in turbulent atmosphere have been derived. The influences of the parameters for turbulent atmosphere and SPGSMP beams on the on-axis and off-axis spectral shift and degree of coherence for SPGSMP beams propagating in turbulent atmosphere have been analyzed, using numerical calculations. The obtained results have potential applications for SPGSMP beams in free-space optical communication and laser lidar.

• 전자통신동향분석
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• 제37권4호
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• pp.81-88
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• 2022

In this study, we investigate the trends and prospects of spatial light modulation (SLM) technology that enables full complex modulation as a next-generation SLM. Current SLM technology, which is used as a key element in holography, augmented reality (AR), XR, and realistic displays, has performance limits that modulate only amplitude or phase. Notably, SLM capable of full complex modulation does not produce diffraction noise, unlike DC and twin image, and thus has a high-efficiency performance. In the future, the application field of next-generation SLM, which can be full-complex modulated, is expected to cover a wide range of holography-AR and-XR devices, optical artificial intelligence, and 6G free space optics communications, which will greatly contribute to the development of a super-realistic metaverse platform and service.

• ETRI Journal
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• 제44권6호
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• pp.966-976
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• 2022

Optical wireless communication, or free space optics, is a promising solution for backhauls in sixth-generation mobile systems. However, the susceptibility of optical links to weather conditions has led to FSO links being furnished with radio frequency (RF) backups. These Hybrid FSO/RF systems provide enhanced link availability but lead to RF resource wastage. Cognitive radio technology, in contrast, is well known for its optimal use of RF resources and may be combined with an FSO link to create a Cognitive Hybrid FSO/RF system. This work uses such a system to analyze a configuration for a mobile backhaul in sixth-generation mobile systems. This configuration can seamlessly coexist with established large scale RF cellular networks. The performance of this configuration is analyzed with respect to outage probability and average bit error by considering the impact of optical channel turbulence, misalignment loss, RF interference, and noise. Mathematical closed-form expressions are verified by simulations.

• 천문학회보
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• 제46권2호
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• pp.55.4-55.4
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• 2021

한국천문연구원에서는 낮은 표면밝기(Low Surface Brightness; LSB)의 천체를 효율적으로 관측할 수 있는 소형(〉30cm) 광시야(〉1°×1°) 광학망원경 및 관측기술 개발을 통한 은하형성 규명 연구를 수행 중에 있다. 이번에 개발한 K-DRIFT pathfinder는 비축 자유곡면 3반사 망원경 시스템(Linear Astigmatism Free-Three Mirror System; LAF-TMS)으로 넓은 시야에서 고품질의 이미지를 효율적으로 얻을 수 있는 광학 설계를 적용하고, 배경 값 변동 요인을 분석하여 가까운 우주의 LSB 천체 관측에 최적화될 수 있도록 하였다. 이번 특별세션에서는 '왜 LSB 우주 탐사를 하고, K-DRIFT를 개발하는지?'에 대해서 소개하고, K-DRIFT pathfinder의 개발 과정, 보현산 천문대에서의 시험관측 결과 소개와 함께, LSB 천체 연구를 위한 맞춤형 시뮬레이션 개발 및 수행 내용을 소개한다.

• 천문학회보
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• 제46권2호
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• pp.56.3-56.3
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• 2021

In a ΛCDM universe, most galaxies are believed to evolve by mergers and accretions. The debris resulting from such processes remains faint and/or diffuse structures, such as tidal streams and stellar halos. Although these structures are a good indicator of the recent mass assembly history of galaxies, they have the disadvantage of being difficult to observe due to their low surface brightness (LSB). To recover these LSB features by reducing the photometric uncertainties introduced by the optics system, we attempt to develop an optimized telescope, called a linear astigmatism free-three mirror system, that minimizes the loss and scattering of light within the telescope. With that prototype, we observe NGC 5907, known as a nearby galaxy with a fabulous loop structure(s), to inspect its performance. After a dedicated data reduction process, including flat-fielding with dark sky flat and sky subtraction, our observation reaches a 1σ surface brightness limit of μlim,r ≃ 28.3 mag arcsec-2 in 10×10 arcsec boxes. We finally identify a single tidal stream that is likely the remnant of a nearly disrupted galaxy. This finding emphasizes that the capability of LSB detection with our telescope is comparable to that of much larger telescopes.