• 대한기계학회논문집
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• 제19권8호
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• pp.2030-2038
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• 1995

In this study, three turbulent flame propagation models are compared using experimentally measured data of a 4 valves/cylinder spark-ignition engine. First two conventional models are B.K model and GESIM combustion model. The burning rates calculated from the two models are compared with the burning rates calculated from measured pressure data using the one-zone heat release analysis. GESIM combustion model predicts burning rates closer to the data acquired from the experiment in wide operating ranges than B-K model does. The third model is refined based on GESIM combustion model by including the effect of flame stretch, turbulent length scale band pass filter and a variable that considers flame size and the area of flame contacting the cylinder wall surface. The refined combustion model predicts burning rates closer to experimental results than GESIM combustion model does. Also, the refined combustion model predicts flame radius close to the experimental result measured by using optical fiber technique.

• 공학교육연구
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• 제4권1호
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• pp.88-98
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• 2001

이 논문은 공업 고등학교의 활성화와 효율화를 위한 새로운 모델로서 학교 자체의 독립성과 다른 학교와의 연계성을 같이 가지고 있는 지능적인 분산 포탈로서의 네트워크 모델을 제안하고 있다. 특히 실습이 많은 공업고등학교에서 동영상 화면을 가지고 있는 시뮬레이션을 무리 없이 활용하기 위해서는 자체의 인트라넷 기능을 수행하면서 필요에 따라 여러 수업 자료를 데이터 베이스로 구축하고 여러 학교가 필요한 자료들을 수업 외의 시간에 학교 데이터 베이스에 적재하여 학내 인트라넷에서 수업시간에 활용할 수 있는 방안을 언급하고 있다. 이러한 구조는 방대한 분산형 데이터 베이스의 활용과 학교 자체의 독립적인 특징을 살릴 수 있어, 물리적인 공업고등학교의 모습과 논리적인 사이버 공업고등학교의 모습이 병합될 수 있을 것이라고 제안하고 있다.

• 천문학회보
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• 제36권2호
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• pp.151.2-151.2
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• 2011

IGRINS (Immersion GRating INfrared Spectrometer) will provide the spectra with high-resolution and an instantaneous spectral coverage of H and K band in NIR region. Therefore, it is expected that the wide coverage of wavelength would make a production of an extensive NIR high-resolution spectra of standard stars as a prior program of IGRINS. As a counter part of these NIR spectra, we have planned to obtain the high-resolution spectra of those standard stars in optical band. These optical high-resolution spectra would give us an opportunity to produce the library of high-resolution stellar spectra covering from optical to NIR band, and to confirm the method to determine the stellar parameters and chemical abundances from the NIR high-resolution spectra. Before using the NIR high-resolution spectra, we have tested the method to determine the stellar parameters by comparing between the observed spectra and the synthetic spectra in optical band. In order to make the synthetic spectra, we have used the Kurucz ATLAS9 model grids and the SYNTH code described by Fiorella Castelli (http://wwwuser.oat.ts.astro.it/castelli/). For the cross-check against the parameters that would be derived from the NIR spectra, the stellar parameters such as effective temperature and surface gravity were determined using the optical spectra of the solar-like stars, as preliminary results.

• 대한전자공학회논문지
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• 제16권3호
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• pp.49-56
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• 1979

A new microwave frequency disriminator in MIC is described which was developed using realization theory appropriate to a transmission line frequency discriminator designed to be used in the VHF range. It is experimentally verified that the discriminator is linear in a 600 MHz bandwith and has VSWR less than 1.2 in that range in agreement with the theoretical model.

• 대한전자공학회논문지
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• 제24권5호
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• pp.747-752
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• 1987

Analysis and design procedures for both symmetrical and non-symmetrical open-circuited interdigital multiple coupled microstrip line structures for applications as wide-band DC blocks/filters have been presented. The design equations, as is the case of other microstrip structures, are based on a simplified TEM model. The experimental results are in good agreement with the theoretically predicted ones.

• 한국통신학회논문지
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• 제32권6B호
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• pp.316-324
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• 2007

In this paper we proposed an energy consumption model for IR-UWB wireless sensor networks. The model takes the advantages of PHY-MAC cross layer design, and we used slotted and un-slotted sleeping protocols to compare the energy consumption. We addressed different system design issues that are responsible to energy consumption and proposed an optimum model for the system design. We expect the slotted sleeping will consume less energy for bursty load than that of the un-slotted one. But if we consider latency, the un-slotted sleeping model performs better than the slotted sleeping case.

• ETRI Journal
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• 제32권1호
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• pp.148-150
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• 2010

This letter presents the design of a compact bandstop filter (BSF) operating at two frequencies. The proposed BSF consists of open-ended stepped impedance resonators (OSIR) and an end-shorted parallel-coupled microstrip line (E-PCML). The OSIRs are used to achieve the impedance-controlled stopband positions. The wide BSF bandwidths are achieved through enhanced coupling of the E-PCML. Explicit design guidelines are derived using a lossless transmission line model. To validate theoretical predictions, a prototype dual-band BSF operating at 900 MHz and 2,100 MHz with fractional bandwidths of 72% and 36%, respectively, is implemented in microstrip.

• 전기전자학회논문지
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• 제24권4호
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• pp.1122-1128
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• 2020

대역 확장(Bandwidth Extension)이란 채널 용량 부족 혹은 이동통신 기기에 탑재된 코덱의 특성으로 인해 부호화 및 복호화 과정에서 대역 제한(band limited)되거나 손상된 협대역 신호(NB, Narrow Band)를 복원, 확장하여 광대역 신호(WB, Wide Band)로 전환 시켜주는 것을 의미한다. 대역 확장 연구는 주로 음성 신호 위주로 대역 복제(SBR, Spectral Band Replication), IGF(Intelligent Gap Filling)과 같이 고대역을 주파수 영역으로 변환하여 복잡한 특징 추출 과정을 거쳐 이를 바탕으로 사라지거나 손상된 고대역을 복원한다. 본 논문에서는 딥러닝 모델 중 오토인코더(Autoencoder)를 바탕으로 1차원 합성곱 신경망(CNN, Convolutional Neural Network)들의 잔차 연결을 활용하여 복잡한 사전 전처리 과정 없이 일정한 길이의 시간 영역 신호를 입력시켜 대역 확장 시킨 음향 신호를 출력하는 모델을 제안한다. 또한 음성 영역에 제한되지 않는 음악을 포함한 여러 종류의 음원을 포함하는 데이터셋에 훈련시켜도 손상된 고대역을 복원할 수 있음을 확인하였다.

• 한국음향학회:학술대회논문집
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• 한국음향학회 2004년도 춘계학술발표대회 논문집 제23권 1호
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• pp.311-314
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• 2004

A new type of high frequency wideband ultrasonic transducer with a separation between a transmitter and a receiver was proposed and its characteristics were simulated using the PSpice model. The piezoelectric ceramic $PbTiO_{3}$ as a transmitter and the piezoelectric copolymer P(VDF-TrFE) as a receiver were used for high sensitivity and wide bandwidth, respectively. The characteristics of a center frequency approximately 40MHz focusing transducer fabricated in this study showed very wide bandwidth which could give an axial spatial resolution better than 30um in the B-mode image for biological tissues.

• 천문학회보
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• 제37권2호
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• pp.83.1-83.1
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• 2012

The galaxy cluster is a good laboratory to test the cosmological model as well as the evolution of galaxies in the dense region. However the lack of wide and deep near-IR datasets has prevented to identify galaxy clusters at z>1. Here we merge a wide, deep near-IR datasets of UKIDSS DXS (J and K bands) and IMS (J band) with the CFHT Legacy Survey (CFHTLS) ugriz catalogue to detect galaxy clusters. We identify candidate galaxy clusters at z>0.8, where the near-IR dataset plays an important role to detect galaxies efficiently. The cluster mass is also estimated based on the cluster richness and the semi-analytical cosmological simulation.