• 제목/요약/키워드: multi resolution analysis

검색결과 414건 처리시간 0.028초

이산 웨이브렛 변환을 이용한 유효 음성 추출에 관한 연구 (A Study on Extracting Valid Speech Sounds by the Discrete Wavelet Transform)

  • 김진옥;황대준;백한욱;정진현
    • 정보처리학회논문지B
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    • 제9B권2호
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    • pp.231-236
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    • 2002
  • 유효한 무성음이 시스템 노이즈와 합성됐을 경우 유효한 무성음 추출에 많은 어려움이 있으나 본 논문에서는 유효한 무성음 추출에 있어 이산 웨이브렛 변환을 이용한 신호 해석 내용을 기반으로 주파수와 그 위치를 블록별로 머징 규칙으로 유효 여부를 결정하기 때문에 노이즈가 많은 환경에서도 유효한 무성음 추출이 가능하다. 머징 알고리즘은 음성만으로도 처리 매개변수를 결정할 수 있고 시스템 잡음에 대하여서도 독립적이기 때문에 유효한 음성을 추출하는데 매우 효과적이다. 실험 결과를 통하여 유효한 음성 추출 처리 과정에서 보다 향상된 결과를 보이고 있으며 특히 고주파 노이즈에 대한 강한 적응력을 제시하고 시스템 구현에도 용이한 시스템 튜닝을 가능케 한다.

웨이블렛 계수와 Hidden Markov Model을 이용한 얼굴인식 기법 (Face Recognition Using Wavelet Coefficients and Hidden Markov Model)

  • 이경아;이대종;박장환;전명근
    • 한국지능시스템학회논문지
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    • 제13권6호
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    • pp.673-678
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    • 2003
  • 본 논문에서는 웨이블렛 계수와 Hidden Markov Model(HMM) 이용한 얼굴인식 알고리즘을 제안 한다. 입력 영상은 이산웨이블렛을 기반으로 한 다행상도 분석기법을 사용하여 데이터 수를 압축한 후, 각각의 해상도에서 얻어진 웨이블렛 계수를 특징벡터로 사용하여 HMM의 모델을 생성한다. 인식단계 에서는 웨이블렛 변환에 의해 생성된 개별대역의 인식값을 더하여 상호 보완함으로써 인식률을 높일 수 있었다. 제안된 알고리즘의 타당성을 검증하기 위하여 기본적 알고리즘인 벡터 양자화(VQ) 기법을 적용한 경우와 기존 얼굴인식에 제안된 DCT-HMM을 이용한 기법과의 인식률 비교를 한 결과, 제안된 방법이 우수한 성능을 보임을 알 수 있었다.

공간좌표로 사상된 GCC 함수의 다 음원에 대한 해석과 음원 위치 추정 방법 (Spatially Mapped GCC Function Analysis for Multiple Source and Source Localization Method)

  • 권병호;박영진;박윤식
    • 제어로봇시스템학회논문지
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    • 제16권5호
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    • pp.415-419
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    • 2010
  • A variety of methods for sound source localization have been developed and applied to several applications such as noise detection system, surveillance system, teleconference system, robot auditory system and so on. In the previous work, we proposed the sound source localization using the spatially mapped GCC functions based on TDOA for robot auditory system. Performance of the proposed one for the noise effect and estimation resolution was verified with the real environmental experiment under the single source assumption. However, since multi-talker case is general in human-robot interaction, multiple source localization approaches are necessary. In this paper, the proposed localization method under the single source assumption is modified to be suitable for multiple source localization. When there are two sources which are correlated, the spatially mapped GCC function for localization has three peaks at the real source locations and imaginary source location. However if two sources are uncorrelated, that has only two peaks at the real source positions. Using these characteristics, we modify the proposed localization method for the multiple source cases. Experiments with human speeches in the real environment are carried out to evaluate the performance of the proposed method for multiple source localization. In the experiments, mean value of estimation error is about $1.4^{\circ}$ and percentage of multiple source localization is about 62% on average.

광섬유 피드 리트로마운트형 분광계 (AN OPTICAL FIBER FEED LITTROW-MOUNTED SPECTROMETER)

  • 배지훈;송재원;윤태석
    • 천문학논총
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    • 제27권3호
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    • pp.87-93
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    • 2012
  • A low-dispersion fiber feed Littrow-mounted grating spectrometer for education was designed and fabricated. The dispersion element is a reflective type blazed grating Edmundoptics NT 46-075 (spatial frequency 600 lines/mm, dimension $30mm{\times}30mm$, blazed angle 8.6 degree). The optical fiber coupler module for optical guiding from telescope to spectrometer is composed of a multi-mode FC connector - FC connector optical fiber patch cord (core/cladding diameter $50{\mu}m/125{\mu}m$) and two 1.25" throw-tube couplers. The lens for collimating and imaging is a general purpose focal length 50 mm camera lens (f/1.8). The device for optical path control is a rectangular prism (size $25mm{\times}25mm$). The imaging camera sensor is a Meade DSI Pro 2 CCD sensor (black and white, $752{\times}582$ pixels and pixel size $8.3{\mu}m{\times}8.6{\mu}m$). Softwares for data logging and analysis consist of Meade Autostar Suite, NIH imagej and Vernier Logger Pro 3. The wavelength coverage range of the spectrometer is 205 nm at central wavelength 550 nm. The wavelength resolution is 1.7 nm.

Airborne Remote Sensing of Evapotranspiration over Rice Paddy

  • Chen, Y.Y.;Liou, Yuei-An
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2003년도 Proceedings of ACRS 2003 ISRS
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    • pp.351-353
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    • 2003
  • We present a retrieval scheme for the remote sensing of evapotranspiration (ET) over rice paddy. To perform the retrieval, high-resolution airborne imagery of multi-spectral visible and thermal infrared data, and ground-based meteorological measurements are utilized. Our ET retrieval scheme is based on the basic principal of surface energy budget, which is a result of balance in longwave and shortwave radiation, latent heat, sensible heat, and energy flux into the ground. To partition the latent and sensible heat fluxes of interest from the energy balance equation, three basic parameters are of most concern, including albedo, surface temperature, and normalized difference vegetation index (NDVI). The NDVI and albedo can be easily derived from the visible and near infrared spectral data, while the surface tem-perature can be determined through the analysis of the infrared data with the Stefan Boltzmann law. From the airborne imagery taken on 28 April 2003, we observe very good dry and wet pixels that can be easily corre-sponded to the radiation and evaporation controlled crite-ria, respectively, and, hence, for the further use in defin-ing the evaporative fraction needed to partition sensible and latent heat fluxes from the net energy flux. The de-rived ET is compared with the in situ measurements.

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멀티스케일 해석을 통한 히스테리시스 고무 마찰 예측 연구 (Predictive Study of Hysteretic Rubber Friction Based on Multiscale Analysis)

  • 남승국;오염락;전성희
    • Tribology and Lubricants
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    • 제30권6호
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    • pp.378-383
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    • 2014
  • This study predicts the of the hysteretic friction of a rubber block sliding on an SMA asphalt road. The friction of filled rubber on a rough surface is primarily determined by two elements:the viscoelasticity of the rubber and the multi-scale perspective asperities of the road. The surface asperities of the substrate exert osillating forces on the rubber surface leading to energy dissipation via the internal friction of the rubber when rubber slides on a hard and rough substrate. This study defines the power spectra at different length scales by using a high-resolution surface profilometer, and uses rubber and road surface samples to conduct friction tests. I consider in detail the case when the substrate surface has a self affine fractal structure. The theory developed by Persson is applied to describe these tests through comparison with the hysteretic friction coefficient relevant to the energy dissipation of the viscoelastic rubber attributable to cyclic deformation. The results showed differences in the absolute values of predicted and measured friction, but with high correlation between these values. Hence, the friction prediction model is an appropriate tool for separating the effects of each factor. Therefore, this model will contribute to clearer understanding of the fundamental principles of rubber friction.

Spectroscopic and Photometric Investigation of BS Cassiopeiae

  • Jeong, Min-Ji;Kim, Chun-Hwey;Hong, Kyeongsoo;Park, Jang-Ho;Yoon, Joh Na;Lee, Jae Woo;Han, Wonyong;Song, Mi-Hwa
    • 천문학회보
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    • 제44권1호
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    • pp.83.3-83.3
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    • 2019
  • New high-resolution spectra and multi-band photometric data of BS Cas were obtained at the Bohyunsan Optical Astronomy Observatory in 2018 and at the Jincheon Station of the Chungbuk National University Observatory in 2011, respectively. We measured the radial velocities (RVs) for both components, and the effective temperature of the more massive star was determined to be $6262{\pm}56K$. In addition, historical light curves showed strong time-dependant light variations at the total eclipse. These variations were modeled by a cool spot on the more massive component. Finally, the physical parameters of BS Cas by a simultaneous analysis of our RV curves with the photometric light curves were presented. Individual masses and radii of both components were deduced as $M_1= 0.59{\pm}0.07M_{\odot}$, $M_2=1.47{\pm}0.15M_{\odot}$, $R_1=0.94{\pm}0.03R_{\odot}$ and $R_2=1.47{\pm}0.05R_{\odot}$.

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A Model to Identify Expeditiously During Storm to Enable Effective Responses to Flood Threat

  • Husain, Mohammad;Ali, Arshad
    • International Journal of Computer Science & Network Security
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    • 제21권5호
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    • pp.23-30
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    • 2021
  • In recent years, hazardous flash flooding has caused deaths and damage to infrastructure in Saudi Arabia. In this paper, our aim is to assess patterns and trends in climate means and extremes affecting flash flood hazards and water resources in Saudi Arabia for the purpose to improve risk assessment for forecast capacity. We would like to examine temperature, precipitation climatology and trend magnitudes at surface stations in Saudi Arabia. Based on the assessment climate patterns maps and trends are accurately used to identify synoptic situations and tele-connections associated with flash flood risk. We also study local and regional changes in hydro-meteorological extremes over recent decades through new applications of statistical methods to weather station data and remote sensing based precipitation products; and develop remote sensing based high-resolution precipitation products that can aid to develop flash flood guidance system for the flood-prone areas. A dataset of extreme events has been developed using the multi-decadal station data, the statistical analysis has been performed to identify tele-connection indices, pressure and sea surface temperature patterns most predictive to heavy rainfall. It has been combined with time trends in extreme value occurrence to improve the potential for predicting and rapidly detecting storms. A methodology and algorithms has been developed for providing a well-calibrated precipitation product that can be used in the early warning systems for elevated risk of floods.

An enhanced incompressible SPH method for simulation of fluid flow interactions with saturated/unsaturated porous media of variable porosity

  • Shimizu, Yuma;Khayyer, Abbas;Gotoh, Hitoshi
    • Ocean Systems Engineering
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    • 제12권1호
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    • pp.63-86
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    • 2022
  • A refined projection-based purely Lagrangian meshfree method is presented towards reliable numerical analysis of fluid flow interactions with saturated/unsaturated porous media of uniform/spatially-varying porosities. The governing equations are reformulated on the basis of two-phase mixture theory with incorporation of volume fraction. These principal equations of mixture are discretized in the context of Incompressible SPH (Smoothed Particle Hydrodynamics) method. Associated with the consideration of governing equations of mixture, a new term arises in the source term of PPE (Poisson Pressure Equation), resulting in modified source term. The linear and nonlinear force terms are included in momentum equation to represent the resistance from porous media. Volume increase of fluid particles are taken into consideration on account of the presence of porous media, and hence multi-resolution ISPH framework is also incorporated. The stability and accuracy of the proposed method are thoroughly examined by reproducing several numerical examples including the interactions between fluid flow and saturated/unsaturated porous media of uniform/spatially-varying porosities. The method shows continuous pressure field, smooth variations of particle volumes and regular distributions of particles at the interface between fluid and porous media.

이어도 해양과학기지 관측 수온과 위성 해수면온도 합성장 자료와의 비교 (Comparison of Multi-Satellite Sea Surface Temperatures and In-situ Temperatures from Ieodo Ocean Research Station)

  • 우혜진;박경애;최도영;변도성;정광영;이은일
    • 한국지구과학회지
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    • 제40권6호
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    • pp.613-623
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    • 2019
  • 지난 수십년 동안 인공위성을 통해 광범위하고 주기적으로 관측된 해수면온도 자료를 사용하여 일별 해수면온도 합성장이 생산되고 있으며 기후변화 감시와 해양 대기 예측 등 다양한 목적으로 활용되어 왔다. 본 연구에서는 지역적인 해역에서 최적화된 활용을 위해 한반도 주변해역에서 해수면온도 합성장 자료의 정확도 평가와 오차 특성 분석을 수행하였다. 2016년 1월부터 12월까지 이어도 해양과학기지 관측 수온 자료를 활용하여 4종의 다중 인공위성 기반 해수면온도 합성장 자료(OSTIA (Operational Sea Surface Temperature and Sea Ice Analysis), OISST (Optimum Interpolation Sea Surface Temperature), CMC (Canadian Meteorological Centre) 해수면온도 및 MURSST (Multi-scale Ultra-high Resolution Sea Surface Temperature))를 비교하여 각 해수면온도 합성장의 정확도를 평가하였다. 이어도 해양과학기지 수온 자료에 대하여 각 해수면온도 합성장은 최소 0.12℃ (OISST)와 최대 0.55℃ (MURSST)의 편차와 최소 0.77℃ (CMC 해수면온도)와 최대 0.96℃ (MURSST)의 평균 제곱근 오차를 나타냈다. 해수면온도 합성장 사이의 상호 비교 결과에서는 -0.38-0.38℃의 편차와 0.55-0.82℃의 평균 제곱근 오차의 범위를 보였으며 OSTIA와 CMC 해수면온도 자료가 가장 작은 오차 특성을 보인 반면 OISST와 MURSST 자료는 가장 큰 오차 특성을 나타내었다. 이어도 해양과학기지와 가장 가까운 지점에서 해수면온도 합성장 자료를 추출하여 시계열을 비교한 결과에서는 이어도 해양과학기지 관측 수온 뿐만 아니라 모든 해수면온도 합성장 자료에서 뚜렷한 계절 변동을 보였으나 봄철 해수면온도 합성장은 이어도 해양과학기지 관측 수온에 비해 과대추정되는 경향이 나타났다.