• 한국지능시스템학회논문지
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• 제7권2호
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• pp.34-42
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• 1997

본 논문은 산업분야의 군사적으로 많이 사용되고 있는 planar shape의 인식을 스펙트럼 분석기를 이용하여 FFT 스펙트럼으로부터 추출된 3차원 특징 벡터와 신경회로망인 fuzzy ARTMAP을 이용하여 시도되었다. 외곽선 정보를 추출하여 이를 원점으로 이동시키고 각 경계점들과 원점들과의 유클리드 거리를 구하여 이를 다시 FFT스펙트럼과 스펙트럼 분석기를 통하여 3차원 특징 벡터를 추출하였다. 이 3차원 데이터는 이동, 회전, 크기에 무관한 값으로 fuzzy ARTMAP에 입력값으로 사용하였다. Fuzzy ARTMAP은 두개의 fuzzy ART 모듈을 가지고 있으며 위에서 구한 특징 벡터들에 의해 학습되고 실험되어 진다.본 논문에 포함된 실험은 4개의 비행기와 4개의 산업부품을 이용하여 잡음이 섞인 shape의 인식에 있엇 제시된 방법이 좋은 인식률을 기록함을 보여주고 있다.

• 천문학회보
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• 제37권1호
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• pp.48.1-48.1
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• 2012

We present the ultraviolet (UV) color-color relation of early-type galaxies (ETGs) in the nearby universe (0.05 < z < 0.12) to investigate the properties of hot stellar populations responsible for the UV excess (UVX). The initial sample of ETGs is selected by the spectroscopic redshift and the morphology parameter from the SDSS DR 7, and then cross-matched with the GALEX far-UV (FUV) and near-UV (NUV) GR6 data. The cross-matched ETG sample is further classified by their emission line characteristics in the optical spectra into quiescent, star-forming, and active galactic nucleus categories. Contaminations from early-type spiral galaxies, mergers, and morphologically disturbed galaxies are removed by visual inspection. By drawing the FUV-NUV (as a measure of UV spectral shape) versus FUV-r (as a measure of UVX strength) diagram for the final sample of -3700 quiescent ETGs, we find that the "old and dead" ETGs consist of a well-defined sequence in UV colors, the "UV red sequence," so that the stronger UVX galaxies should have a harder UV spectral shape systematically. However, the observed UV spectral slope is too steep to be reproduced by the canonical stellar population models in which the UV flux is mainly controlled by age or metallicity parameters. Moreover, 2 mag of color spreads both in FUV-NUV and FUV-r appear to be ubiquitous among any subsets in distance or luminosity. This implies that the UVX in ETGs could be driven by yet another parameter which might be even more influential than age or metallicity.

• 한국음향학회지
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• 제14권3호
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• pp.90-96
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• 1995

잡음섞인 관측데이타로부터 AR 모수를 추정하는 방법을 제안하였다. AP 방법이라고 이름붙인 이 방법은 단순하고도 신뢰성있는 적응예측기를 이용하려는 시도의 산물이다. 잡음섞인 입력수열로부터 계산된 AR 모수의 추정치보다 예측수열로부터 계산된 AR 모수의 추정치가 원래의 모수에 스펙트럼상의 거리가 더 가깝다는 것을 이론적으로 증명하였다. 실제 음성 신호와 칼만필터를 사용한 실험결과도 이론과 일치함을 보였다. 대략적으로, AP방법으로 계산된 추정치를 사용하였을때의 잡음감쇠성능은 잡음섞인 입력수열로부터 계산된 AP 모수의 추정치를 사용하였을때보다는 우수하였고, EM반복법에 의한 추정치를 사용하였을때보다는 약간 못한 것으로 나타났다. 그러나, 제안된 방법은 그 단순성으로 인하여 경우에 따라 더 복잡한 다른 방법의 대안으로 사용될 수 있을 것이다.

• 대한의용생체공학회:의공학회지
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• 제16권4호
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• pp.395-402
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• 1995

자기공명 영상 시스템에서 영상을 얻고자 하는 물체내의 자화율 차이는 복셀내의 스핀들의 위상을 변화시킨다. 또한 스핀들 상호간의 위상변화로 인하여 영상 신호는 감쇄된다. 이러한 신호 세기의 감쇄는 자기공명 영상분야에서 자화율 효과라 알려져 왔고 이런 효과를 억제시키거나 또는 이용하는 연구가 심도있게 논의되어왔다. 본 논문에서 자화율 효과로 인한 신호의 변화를 분석할 수 있는 새로운 스펙트럼 분해법과 영상법을 제안하였다. 그리고 자화율 스펙트럼 분해법을 위한 펄스시퀀스를 개발하였고, 이것을 상자성(paramagnetic) 성질 때문에 자화율 효과가 생기는 정맥영상에 적용하였다. 컴퓨터 모의 실험과 팬텀(phantom)을 대상으로 한 실험 결과로 스펙트럼 분해법의 타당성을 보였다.

• 천문학회보
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• 제36권2호
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• pp.55.1-55.1
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• 2011

Luminous infrared galaxies (LIRGs; $L_{IR}$ > ${10^{11}}_{Lsun}$) are the most powerful objects in the local Universe. Previous work suggested that dust re-processing of starburst and/or active galactic nuclei (AGN) activity, triggered by galaxy interactions, is responsible for their enormous infrared emission. To understand the nature of LIRGs, it is essential to determine their spectral types. Optical spectral types of 115 ultraluminous infrared galaxies in the southern sky are presented using CTIO observations. The AGN fraction is on average 50% and increases with infrared luminosity. Near-infrared spectral types of 36 LIRGs are also presented based on AKARI observations. In the sample, 12 optically elusive buried AGNs are found. To investigate the evolutionary sequence of LIRGs, star formation histories of ~6000 LIRGs in the SDSS and IRAS/AKARI matched sample are derived by comparing observed optical spectra and stellar population models. AGN-dominated LIRGs are currently massive relative to starburst-dominated LIRGs, which originates from an enhancement of star formation at intermediate-ages. For ~1100 early-type LIRGs, optical and NIR fundamental planes (FPs) are constructed. The FP of LIRGs is significantly different from that of normal early-type galaxies, but the difference is minimized in low luminous and AGN-like LIRGs. These findings support that the importance of AGN is growing as infrared luminosity increases and that LIRGs follow at least in the high mass regime the standard evolutionary scenario: starburst LIRGs evolve into AGN LIRGs and finally into normal early-type galaxies.

• 한국음향학회:학술대회논문집
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• 한국음향학회 1994년도 FIFTH WESTERN PACIFIC REGIONAL ACOUSTICS CONFERENCE SEOUL KOREA
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• pp.912-918
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• 1994

Poor speech intelligibility in an air traffic control room is frequently a result of many, quite different causes and occasionally leads to complaints of the controller personnel. The paper describes a sequence of successful tasks performed in a local control room. The initial measurements included an investigation of the background noise (caused by fans, air condition, computer and radar equipment) and performance checks of the electronic audio and communication equipment with respect to the audio transmission behavior. The spectral composition of the noise as well as the characteristics of the audio communication path between the controllers and the pilots(which showed a loss of spectral information in the audio band due to built-in notch filters for the suppression of control tones) required adaptations of the amplitude behavior of the amplifiers through user adjustable tone controls. The radar console fans, which contributed significantly to the overall noise floor of the room, underwent a substantial reconstruction by replacing the tight mounting with an elastic double suspension, reducing the noise level by 50%. Finally, a possible source of untimely fatigue of the controllers during their working hours has been found in strong spectral components of the noise above the audio band, radiated by numerous video monitors in the control through vibrating components excited by the line frequency of the video signal.

• 대한조선학회논문집
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• 제39권4호
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• pp.1-10
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• 2002

초기쇄파의 수치모사에는 지금까지 경계적분법이 주로 쓰여왔고, 이 방법은 과도한 계산시간의 문제를 제외하고는 어느 정도 성공적이라고 할 수 있다. 본 논문에서는 쇄파실험을 수치모사하기 위한 새로운 수치기법을 보였다. 이 수치기법은 고차 스펙트럴/경계요소법과 경계적분법을 순차적으로 사용하며, 계산시간을 현저히 줄여준다. 조파 및 파 에너지 집중과정은 고차 스펙트럴/경계요소법에 의해 효율적으로 수치모사되고, 파의 전복과정만이 경계적분법에 의해 계산된다. 계산예에서 높은 입자속도와 가속도 등 쇄파의 두드러진 특성이 보여졌다.

• 한국자기공명학회논문지
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• 제10권1호
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• pp.59-73
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• 2006

Spin-lattice relaxation pathway of $CH_2$ spin system by two dimensional NOESY sequence has been discussed. Two-dimensional spectra governed by dipolar relaxation mechanism were simulated in term of transfer mode, the generalization of conventionally used magnetization mode in one dimension. The transfer matrix directly related to the Redfield relaxation matrix can be constructed by the multiplet of transfer mode. The observable relaxation transfer modes causes to variation of the off-diagonal signal intensity of phase sensitive NOESY spectra from which variable spectral density can be extracted with simple group theoretical calculation. The variation of the J-coupling peak intensity as a function of the mixing time in 2-D spectra for $n-Undecane-5-^{13}C$ and Bromoacetic $2-^{13}C$ acid has been theoretically traced.

• 제어로봇시스템학회:학술대회논문집
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• 제어로봇시스템학회 2001년도 ICCAS
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• pp.92.6-92
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• 2001

MSC is being developed to be installed on KOMPSAT(Korea Multi-Purpose Satellite-II and to provide high resolution multi-spectral. MSC consists of three main subsystems. One is EOS(Electro-Optics Subsystem), another is PMU(Payload Management Unit) and the other is PDTS(Payload Data Transmission Subsystem). There is an SBC(Single Board Computer) in the PMU to control all MSC subsystems. SBC incorporates Intel 80486 as a main processor and VxWorks as a real-time operating system. SBC software consists of four main tasks and several modules to deal with all control information for imaging and all the state of health telemetrv data, and to perform interface with another MSC units. SBC software also has to handle a lot of commands in order for MSC to perform his mission. One mission command consists of a series of related commands, which are In be executed in the designated sequence, with a specified time ...

• 대한자기공명의과학회:학술대회논문집
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• 대한자기공명의과학회 2003년도 제8차 학술대회 초록집
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• pp.87-87
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• 2003

Purpose： To determine the motor cortex dysfunction in hemiparetic patients due to deep intracerebral hematoma, authors peformed proton magnetic resonance spectroscopy (1H MRS) for the evaluation of biochemical changes in the cortex on affected hemisphere according to axonal injury at the level of internal capsule. Materials and methods： Ten control subjects and 14 patients with documentable hemiparesis of varying severity hemiparesis were included. All the hemiparesis was caused by deep intracerebral hematoma (putaminal and thalamic hemorrhage). In vivo 1H MRS study was performed on a 3T MRI/MRS system using STEAM sequence. As a single-voxel technique, Spectral parameters were： 20 ms TE, 2000 ms TR, 128 averages, 2500 Hz spectral width, and 2048 data points.