• 한국지능시스템학회논문지
• /
• 제14권6호
• /
• pp.674-677
• /
• 2004

본 논문에서는 심볼간의 간섭이 존재하는 채널에서 고정 지연 값을 가지는 트리검색 신호검출기의 효율적인 구성방법을 다룬다. 이 접근방법은 효율적인 다차원 신호공간 분할에 기반을 두고 있다 다차원 공간에서의 Voronoi 다이어그램 (VoD)과 Delaunay 분할 (DT)이 신호검출 알고리즘의 구현에 적용된다 제안된 방식에서는 VOD/DT에 포함되어 있는 기하학적인 정보를 활용하여 관찰된 순차적인 신호의 상대적인 위치가 결정되며 이러한 방식이 구현치 복잡도를 감소시키는 장점이 있음을 보인다. 구체적인 구성 절차가 심볼간의 간섭이 존재하는 통신채널에서의 예를 가지고 논의되며 시뮬레이션 결과가 논의된다.

• 천문학회보
• /
• 제42권2호
• /
• pp.53.2-53.2
• /
• 2017

Stochasitc gravitational wave background (SGWB) is expected to be contributed by primordial sources (e.g. inflation signature) and astrophysical sources (e.g., incoherent superposition of a large numbers of compact binary inspirals throughout in the Universe). Theoretically, SGWB is predicted to span in a broad frequency range between less than nHz up to kHz. Many gravitational-wave (GW) detectors such as LIGO or LISA aim to detect or constrain SGWB in different frequency band that is most sensitive for each detector. In this talk, we focus on the prospectives of constraining the energy density of SGWB between 0.1-10 Hz. We introduce the characteristics of SGWB and representative models for primordial and astrophysical sources. Then, we propose a signal extraction scheme to detect SGWB using one or several omni-directional GW detectors such as SLGT(Superconducting Low-frequency Gravitational-wave Telescope). Considering SLGT sensitivity, we discuss how to observe SGWB in 0.1-10 Hz if we have SLGT network. Finally, we highlight interesting SGWB models that can be constrained in 0.1-10 Hz with SLGT.

• Nuclear Engineering and Technology
• /
• 제52권2호
• /
• pp.456-460
• /
• 2020

In this research, a radiation detection backpack to be used discreetly or by a wide range of users was developed using array silicon-photomultiplier (SiPM) and CsI (Tl), and its characteristics were evaluated. The R-squared value, which indicates the responsiveness of a detector based on the signal intensity, was determined to be 0.981, indicating a good linear responsivity. The energy resolutions for gamma radiation energies of Co-57 (122 keV), Ba-133 (356 keV), Cs-137 (662 keV), and Co-60 (1332 keV) were found to be 13.40, 10.50, 6.77, and 3.16%, respectively. These results confirm good energy resolution characteristics. Furthermore, in the case of mixed sources, the gamma radiation peaks were readily distinguishable, and the R-squared value for energy linearity was calculated to be 0.999, demonstrating an exceptional energy linearity. Further research based on the results of this study would enable the commercialization of lightweight SiPM-based wireless radiation detection backpacks that can be used for longer durations by replacing the photomultiplier tube, which is mainly used as the optical sensor in existing radiation detection backpacks.

• Current Optics and Photonics
• /
• 제3권6호
• /
• pp.577-582
• /
• 2019

We report on a continuous-wave (cw) optical parametric oscillator (OPO) optimized for mid-infrared emission above 5.0 ㎛. The OPO is based on a magnesium-oxide-doped periodically poled LiNbO₃(MgO:PPLN) crystal with a fan-out grating design. A linear two-mirror cavity resonating both at the pump and signal wavelengths is stabilized to the pump laser by using the modified Pound-Drever-Hall (PDH) method. The idler wavelength is continuously tunable from 4.7 ㎛ up to 5.3 ㎛ by varying the poling period of the fan-out grating crystal. Pumped by a diode-pumped solid state (DPSS) laser with a power of 1.1 W at 1064 nm, the maximum idler output power is measured to be 5.3 mW at 4.8 ㎛. The output power above 5.0 ㎛ is reduced to the hundreds of ㎼ level due to increased absorption in the crystal, but is stable and strong enough to be measured with a conventional detector.

• 천문학회보
• /
• 제35권2호
• /
• pp.58.1-58.1
• /
• 2010

Telescope Array (TA) experiment in Utah, USA, observes ultrahigh-energy cosmic rays (UHECRs); UHECRs refer cosmic rays with energy above $10^{18}eV$. Using COSMOS and CORSIKA, we have produced a library of over 1000 thinned extensive air shower (EAS) simulations with the primary energies ranging from $10^{18.5}eV$ to $10^{20.25}eV$ and the zenith angle of primary cosmic ray particle from $0^{\circ}$ to $45^{\circ}$. Here, we present the energy spectrum of particles arriving at the ground. We have also calculated the detector response evaluated using GEANT4 simulations. Here, we discuss S(800), i.e. the signal at a distance of 800 m from the shower core, as the primary energy estimator.

• 대한전자공학회논문지SD
• /
• 제40권12호
• /
• pp.24-30
• /
• 2003

본 논문에서는 첨두 검출기의 구조를 개선함으로써 정착시간(settling time)을 더욱 단축시킬 수 있는 적응형 기준레벨자동 발생회로를 제안했다. 제안한 기준레벨 자동 발생회로에 대해 비슷한 정착시간을 설정하였을 때에 오차전압비율이 기존 구조에 비해 절반 이하로 줄일 수 있어 정착시간을 상당량 개선할 수 있음을 해석을 통해 밝혔다. 아울러 상용 파운드리(foundry)를 이용하여 1.25G EPON 시스템용 버스트 모드기준레벨 자동 발생회로를 설계한 결과 동적 영역(dynamic range)이 40㏈인 입력신호에 대해 6㎱ 라는 매우 짧은 시간 이내에 기준 레벨을 생성해 내는 결과를 얻을 수 있었다.

• 한국전자파학회:학술대회논문집
• /
• 한국전자파학회 2003년도 종합학술발표회 논문집 Vol.13 No.1
• /
• pp.208-212
• /
• 2003

An airborne radar is an essential aviation electronic system of the helicopter to perform various missions in all-weather environments. This paper presents the conceptual design results of the multi-mode pulsed Doppler radar system testbed model for helicopter. Due to the inherent flight nature of the hovering vehicle which is flying in low-altitude and low speed, as well as rapid maneuvering, the moving clutters from the platform should be suppressed by using a special MTD (Moving Target Detector) processing. For the multi-mode radar system model design, the flight parameters of the moving helicopter platform were assumed: altitude of 3 Km, average cruising velocity of 150knots. The multi-mode operation capability was applied such as short-range, medium-range, and long-range depending on the mission of the vehicle. The nominal detection ranges is 30 Km for the testbed experimental model, but can be expanded up to 75 Km for the long range weather mode. The detection probability of each mode is also compared in terms of the signal-to noise ratio of each mode, and the designed radar system specifications ate provided as a design results.

• 항공우주기술
• /
• 제8권2호
• /
• pp.160-169
• /
• 2009

본 논문은 검출기의 비선형 모델을 바탕으로 유도된 영상 신호-잡음비(Image SNR)[1]의 분포도를 시뮬레이션을 통하여 검증하고, 선형/비선형 이득값들의 변화에 따른 분포도의 특성을 분석한다. 특히, 이득값들의 변화에 따른 분포도의 영향은 운영중인 위성 카메라의 잡음 특성 변화에 상관없이 이득값들에 의한 영상 신호-잡음비 변화 가능성을 보여준다. 마지막으로 본 논문은 영상 신호-잡음비 분포도를 이용하여 운영 변수(누적횟수, 노출시간) 선정과 관련된 최적화 방법에 대한 예시를 제시함으로써, 유도된 분포도의 유용성을 확인한다.

• 한국조명전기설비학회지:조명전기설비
• /
• 제10권5호
• /
• pp.101-107
• /
• 1996

본 연구에서는 대규모 공장과 같은 수변전계통의 전압개선을 위한 전압보상설비의 특성을 해석하는 기법을 제시했다. 보상설비는 전력전자 기술을 이용한 SVC에 대해서 전기적인 과도특성 해석에 가장 정확안 S/W중 하나인 EMTP를 이용하여 TCR전류, 전압 및 점호특성 등을 분석하였다. 이러한 해석기법은 전압개선의 필요성이 높은 제철공장과 같은 대규모 공장의 수변전계통에서 외란에 대한 SVC의 전압개선 특성효과를 분석하는데 유용함을 보였다.

• 대한기계학회:학술대회논문집
• /
• 대한기계학회 2008년도 추계학술대회A
• /
• pp.322-326
• /
• 2008

In this paper, we have studied the images which have been reconstructed by using combination of images acquired by the variation of operating frequency. When inner images have been reconstructed, they have been superposed by the surface state effect. In this case, the images of the phase object can be enhanced by the contrast of inner images. There is a kind of specimen, one is a reference block having 1/4T, 1/2T, 3/4T side drilled holes as main run piping material of the steam generator in nuclear power plants. It has been shown that the two results of defect shapes have better than before in this processing and phase contrast grow about twice. And we have constructed the acoustic microscope by using a quadrature detector that enables to acquire the amplitude and phase of the reflected signal simultaneously. Further more we have studied the reconstruction method of the amplitude and phase images, the enhancement method of the defect images' contrast.