• 한국해양공학회지
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• 제8권1호
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• pp.62-70
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• 1994

In order to estimate the detection range of a active SONAR system, the SONAR equation is commonly used. In this paper, an algorithm to calculate detection range in active SONAR system as function of SONAR depth and target depth is presented. For given SONAR parameters and environment, the transmission loss and background level are found, signal excess is computed. Using log-normal distribution, signal excess is converted to detection probability at each range. Then, the detection range is obtained by integrating the detection probability as function of range for each depth. The proposed algorithm have been applied to the case of omni-directional source with center frequency 30Hz for summer and winter sound profiles. It is found that the optimal search depth is the source depth since the detection range increase at source depth where the signal excess is maximized.

• 한국군사과학기술학회지
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• 제15권5호
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• pp.630-634
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• 2012

It is very important to place receiver in multistatic sonar. Inefficient placement of the receiver reduce detection probability and to increase the probability of detection should be used more receivers. Therefore, detection of targets in searching area, detection performance of limited receiver depends on how to place. Through the optimized receiver placement, detection area between each sonar as much as possible avoid duplication, as optimization, the minimum receiver can be maintained detection performance. In this paper we prove mathematical verification of maximum signal excess value based on sonar placement and we calculate a signal excess value by using computer simulations and suggest optimal sonar placement.

• 대한기계학회:학술대회논문집
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• 대한기계학회 2002년도 학술대회지
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• pp.353-356
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• 2002

Planar laser induced fluorescence(PLIF) has been widely used to obtain two dimensional fuel distribution. Preliminary investigation was performed to measure quantitative air excess ratio distribution in an engine fueled with LPG. It is known that fluorescence signal from acetone as a fluorescent tracer is less sensitive to oxygen quenching than other dopants. Acetone was excited by KrF excimer laser (248nm) and its fluorescence image was acquired by ICCD camera with a cut-of filter to suppress Mie scattering from the laser light. For the purpose of quantifying PLIF signal, an image processing method including the correction of laser sheet beam profile was suggested. Raw images were divided by each intensity of laser energy and profile of laser sheet beam. Inhomogeneous fluorescence images scaled with the reference data, which was taken by a calibration process, were converted to air excess ratio distribution. This investigation showed instantaneous quantitative measurement of planar air excess ratio distribution for gaseous fuel.

• 천문학회보
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• 제39권2호
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• pp.54-54
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• 2014

We use dense redshift surveys of nine galaxy clusters at z ~ 0.2 to compare the galaxy distribution in each system with the projected matter distribution from weak lensing. By combining 2087 new MMT/Hectospec redshifts and the data in the literature, we construct spectroscopic samples within the region of weak-lensing maps of high (70-89%) and uniform completeness. With these dense redshift surveys, we construct galaxy number density maps using several galaxy subsamples. The shape of the main cluster concentration in the weak-lensing maps is similar to the global morphology of the number density maps based on cluster members alone, mainly dominated by red members. We cross correlate the galaxy number density maps with the weak-lensing maps. The cross correlation signal when we include foreground and background galaxies at 0.5zcl < z < 2 zcl is 10 - 23% larger than for cluster members alone at the cluster virial radius. The excess can be as high as 30% depending on the cluster. Cross correlating the galaxy number density and weak-lensing maps suggests that superimposed structures close to the cluster in redshift space contribute more significantly to the excess cross correlation signal than unrelated large-scale structure along the line of sight. Interestingly, the weak-lensing mass profiles are not well constrained for the clusters with the largest cross correlation signal excesses (>20% for A383, A689 and A750). The fractional excess in the cross correlation signal including foreground and background structures could be a useful proxy for assessing the reliability of weak-lensing cluster mass estimates.

• 융합신호처리학회논문지
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• 제14권2호
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• pp.95-98
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• 2013

LMS(Least Mean Square)알고리즘은 강인성, 높은 추적성, 구현의 단순성 때문에 아직도 많이 사용되는 알고리즘이다. 하지만, LMS알고리즘은 비균일적인 수렴율과 EMSE(Excess mean square error)사이에 trade-off를 가진다. 이러한 단점을 극복하기 위해, 많은 가변 스텝 사이즈 알고리즘이 연구되고 있다. 빠른 수렴속도를 위하여 복잡한 가변스텝 방식을 사용 하는데 많은 계산량을 필요로 한다. IGC(Instantaneous Gain Control) 알고리즘은 원신호와 잡음신호의 순시이득값을 사용하여 계산량은 줄이고 높은 성능을 유지한다. 하지만 IGC 알고리즘은 이득값 계산시 log함수에 의해 실행시간이 오래 걸리는 단점을 가진다. 제안하는 변형 IGC알고리즘은 실행시간을 지연하는 log 함수를 제거하여, 실시간 소음제거 처리에 맞게 변형하여 성능 개선을 이룰 수 있었다.

• 한국자동차공학회논문집
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• 제12권1호
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• pp.74-82
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• 2004

Planar laser-induced fluorescence(PLIF) has been widely used to obtain two dimensional fuel distribution. Acetone PLIF is chosen because fluorescence signal from acetone as a fluorescent tracer is less sensitive to oxygen quenching than other dopants. Acetone PLIF is applied to measure quantitative air excess ratio distribution in an engine fueled with LPG. Acetone is excited by KrF excimer laser (248nm) and its fluorescence image is acquired by ICCD camera with a cut-off filter to suppress Mie scattering from the laser light. For the purpose of quantifying PLIF signal, an image processing method including the correction of laser sheet beam profile is suggested. Raw images are divided by each intensity of laser energy and profile of laser sheet beam. Inhomogeneous fluorescence images scaled with the reference data, which is taken by a calibration process, are converted to air excess ratio distribution. This investigation shows instantaneous quantitative measurement of planar air excess ratio distribution for gaseous fuel.

• 한국광학회:학술대회논문집
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• 한국광학회 1999년도 제16회 광학 및 양자전자 학술발표회Proceedings of 16th Optics and Quantum Electronics Conference, 1999
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• pp.226-227
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• 1999

In the fiber-optic gyroscope employing the erbium-doped fiber source, the source excess noise was subtracted through a signal processing to improve the gyroscope sensitivity . As the result, we obtained the improvement of 14 dB(electrical) at the proper frequency, which was measured from the noise floor spectrum . In addition the random walk coefficient in the gyro output was reduced by about factor of three.

• 한국음향학회지
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• 제25권8호
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• pp.395-402
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• 2006

능동-소나를 이용하여 수중표적을 탐지하는데 있어 소나탐지 성능은 잔향음에 많은 제한을 받는다. 해상풍은 해양에서 기포 형성에 중요한 역할을 한다. 그리고 기포는 유효한 산란체로서 잔향음에 기여한다. 본 연구에서는 중주파수 선저 고전형 능동소나를 운용 시 풍성기포가 음파전달에 미치는 영향을 연구하였다. 주파수 5, 7.5, 10kHz에 대해 기포층을 고려한 음원수심 3, 5, 10m에서의 능동 신호초과비 (Active Signal Excess:ASE)를 계산하였다. 해수면 부근의 음속변화는 해수면 잔향음 준위를 증가시키며, 능동 신호초과비를 변화시킨다 풍속이 10m/s에서 해수면 부근의 최대 탐지거리가 3km 이상 감소하였다. 그 원인은 풍성기포에 의한 해수면 방향으로의 굴절로 분석되었다.

• 한국통신학회논문지
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• 제34권8C호
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• pp.756-763
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• 2009

LMS알고리즘은 잡음이 섞인 신호로부터 원 신호를 복원하는데 자주 사용된다. 이 LMS알고리즘의 주된 결점은 음성 신호 파워에 따라 선형적으로 EMSE(Excess Mean Square Error)가 증가한다. 그 결과 최적의 값에서 큰 EMSE 때문에 성능의 효율성이 떨어진다. 이러한 결점은 적은 스텝사이즈를 선택함으로서 해결 할 수 있지만, 수렴율이 늦어지는 단점이 있어, 빠른 수렴율과 낮은 EMSE를 동시에 만족할 수 있는 값이 필요하다. 본 논문에서는 IGC(lnstantaneous Gain Control) 알고리즘을 음성신호가 존재하는 경우에서 제안한다. 시뮬레이션은 음성신호와 가우시안 잡음을 이용하여 수행하였고, 수렴율, 잡음제거, 그리고 EMSE에서 LMS알고리즘보다 IGC알고리즘이 우수하다는 것을 보인다.

• 천문학회보
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• 제44권1호
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• pp.35.1-35.1
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• 2019

We present a statistical analysis on the spin-orbit alignment of dark matter halo pairs in cosmological simulations. The alignment is defined as the angular concurrence between the halo spin vector (${\vec{S}}$) and the orbital angular momentum vector (${\vec{L}}$) of the major companion. We identify interacting halo pairs with the mass ratios from 1:1 to 1:3, with the halo masses of 10.8 < $Log(M_{halo}/M_{sun}$) < 13.0, and with the separations smaller than a sum of their virial radii ($R_{12}<R_{1,vir}+R_{2,vir}$). Based on the total energy ($E_{12}$), the pairs are classified into flybys ($E_{12}$ > 0) and mergers ($E_{12}{\leq}0$). By measuring the angle (${\theta}_{SL}$) between ${\vec{S}}$ and ${\vec{L}}$, we confirm a strong spin-orbit alignment signal such that the halo spin is preferentially aligned with the orbital angular momentum of the major companion. We find that the signal of the spin-orbit alignment for the flyby is weaker than that for the merger. We also find an unexpected excess signal of the spin-orbit alignment at $cos{\theta}_{SL}{\sim}0.25$. Both the strength of the spin-orbit alignment and the degree of the excess depend only on the environment. We conclude that the halo spin is determined by the accretion in a preferred direction set by the ambient environment.