• 한국음향학회지
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• 제39권2호
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• pp.113-119
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• 2020

자동차에서의 모터 사용 증가로 자동차 실내 음질(sound quality) 향상을 위해 모터 소음이 주요 관심사이다. 본 연구의 목적은 부하변화에 따른 모터 소음 성능을 나타낼 수 있는 인자를 제안하는 것이다. 이를 위하여, 파워스펙트럼과 라우드니스가 소음 성능을 나타내는데 적합하지 않음을 확인하였고, 브러쉬 마찰 성분과 관련된 부분라우드니스(PN_B)와 토크 리플 성분과 관련된 부분라우드니스(PN_R)가 소음 성능을 나타내는 인자로 파악되었다. 그리고 PN_B와 PN_R를 이용하여 부하에 따른 모터 소음의 변화 특성을 나타내기 위한 방법으로 모터 소음 성능 곡선을 제안하였다. 이 곡선은 소음 제어, 모터 선정 및 시스템 개선을 위한 가이드로 활용될 것으로 기대된다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2009년도 제33회 추계학술대회논문집
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• pp.231-235
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• 2009

본 연구의 목적은 실제로 서인천 발전본부에서 운용하고 있는 GE 7FA+e DLN 2.6 가스터빈 연소기의 연소특성과 배기배출물에 대한 제어 연구를 소개하고 모형 가스터빈 연소기의 연소동특성 및 연소불안정 현상을 확인하고자 한다. 모형 연료노즐은 실제의 1/3 크기로 상사하여 제작되었고, 실제 노즐과 동일한 각도의 2단 스월러(swirl vane)를 가지고 있다. Plenum과 연소기의 형상은 실 가스터빈과 유사한 음향학적 특성을 가질 수 있도록 설계되었고 실험은 공기온도, 노즐출구 속도, 당량비, 연소실 길이를 변수로 이루어졌으며, 그 결과 연소실의 연소불안정 mode는 각각의 실험 변수에 따라서 연소실의 공진주파수의 영향, 연소온도와 공기-연료 혼합기 분포에 의해서 mode가 전이되는 현상을 확인하였다.

• 한국초전도ㆍ저온공학회논문지
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• 제22권2호
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• pp.38-43
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• 2020

This paper presents comparative research on characteristics of air-cored and iron-cored high-temperature superconductor (HTS) field winding synchronous motors. The 100 kW air-cored model is designed analytically by Spatial Harmonic Method, and based on this model, the iron-cored model having the same output power is designed for comparison. Due to the substantial difference of permeability property between air and iron-core, there is a difference of magnetic field magnitude and angle with respect to the HTS tape c-axis, resulting in a different critical current of the field winding considering the anisotropic property of HTS tape. For a detailed comparison between two models, the following key motor characteristics are calculated through the Finite Element Method (FEM) simulation: 1) critical current; 2) HTS wire length; and 3) torque characteristics. From the simulation results, it can be confirmed that the critical current value of the iron-cored model increases by 33 %. Also, in the case of the superconducting wire consumption, those of the iron-cored and air-cored models are 95.3 m and 815.6 m, respectively. So the wire usage can be reduced to about 88 % by using iron core. However, in terms of torque characteristics, the torque ripple of the iron-cored model is about twice as large as that of the air-cored model, which may be a disadvantage on vibration and acoustic noise.

• 전자공학회논문지SC
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• 제48권5호
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• pp.1-6
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• 2011

LED(Light Emitting Diode) 소자는 현대 기술의 발달로 형광등이나 전구보다 수명이 길고 전력소모가 작으며 제어가 쉽다는 장점을 가지고 있다. 이러한 이유로 LED 소자를 이용한 조명이 많이 사용되고 있다. 최근 LED 소자의 고속응답특성을 이용한 통신기법인 가시광통신(Visible Light Communication, 이하 VLC)이 주목받기 시작하였다. VLC의 경우 전파를 사용하지 않아 주파수 할당이 필요가 없으며, 데이터전송에 ISM(Industrial Scientific Medical band)과 같은 간섭 또한 존재하지 않는다. 그렇기 때문에 VLC에 관한 연구 결과가 많이 나오고 있다. 본 논문에서는 기존의 LED 조명을 사용한 VLC와 수중환경에서의 VLC에 대한 survey를 진행하고 활용방법을 살펴보았다.

• 전자공학회논문지SC
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• 제42권3호
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• pp.33-40
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• 2005

심해저 자원의 확보를 위해서는 먼저 해양환경을 탐사하고 관측해야하며 이를 위해서 계측장비를 해저에 위치시키고 탐사가 끝난 후 회수하는 방법을 사용하는데 이 경우 계절변화에 따른 염분의 농도 및 온도 변화로 다양한 형태의 외란성 노이즈가 발생하여 제어 안정성과 수중통신에 대한 신뢰성이 떨어지고 있다. 그래서 기존의 제어방법은 수신된 제어정보를 하드웨어적인 방법으로 식별하고 기준 정보와 비교하며 이 과정을 수차례 반복하여 획득한 데이터를 제어정보로 활용하고 있다. 이는 제어의 신뢰성이 중요시 되는 시스템에서는 제어안정성 및 효율성이 떨어지고 있다. 따라서 본 논문에서는 해양환경 변화에 대한 제어안정성 및 동작신뢰성을 향상시킨 수중 탐측장비 회수용 원격 이탈제어 시스템을 제안하고자 한다. 그리고 제어알고리즘 및 원격 이탈제어 시스템의 적합성을 실험을 통하여 확인하였다.

• 천문학회지
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• 제44권6호
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• pp.217-234
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• 2011

We present two large cosmological N-body simulations, called Horizon Run 2 (HR2) and Horizon Run 3 (HR3), made using $6000^3$ = 216 billions and $7210^3$ = 374 billion particles, spanning a volume of $(7.200\;h^{-1}Gpc)^3$ and $(10.815\;h^{-1}Gpc)^3$, respectively. These simulations improve on our previous Horizon Run 1 (HR1) up to a factor of 4.4 in volume, and range from 2600 to over 8800 times the volume of the Millennium Run. In addition, they achieve a considerably finer mass resolution, down to $1.25{\times}10^{11}h^{-1}M_{\odot}$, allowing to resolve galaxy-size halos with mean particle separations of $1.2h^{-1}$Mpc and $1.5h^{-1}$Mpc, respectively. We have measured the power spectrum, correlation function, mass function and basic halo properties with percent level accuracy, and verified that they correctly reproduce the CDM theoretical expectations, in excellent agreement with linear perturbation theory. Our unprecedentedly large-volume N-body simulations can be used for a variety of studies in cosmology and astrophysics, ranging from large-scale structure topology, baryon acoustic oscillations, dark energy and the characterization of the expansion history of the Universe, till galaxy formation science - in connection with the new SDSS-III. To this end, we made a total of 35 all-sky mock surveys along the past light cone out to z = 0.7 (8 from the HR2 and 27 from the HR3), to simulate the BOSS geometry. The simulations and mock surveys are already publicly available at http://astro.kias.re.kr/Horizon-Run23/.

• Journal of Mechanical Science and Technology
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• 제18권2호
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• pp.185-192
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• 2004

The aeroacoustic characteristics of a centrifugal fan for a vacuum cleaner and its noise reduction method are studied in this paper. The major noise source of a vacuum cleaner is the centrifugal fan. The impeller of the fan rotates at over 30000 rpm, and generates very high-level noise. It was revealed that the dominant noise source is the aerodynamic interaction between the rotating impeller and stationary diffuser. The directivity of acoustic pressure showed that most of the noise propagates backward direction of the fan-motor assembly. In order to reduce the high tonal sound generated from the aerodynamic interaction, unevenly pitched impeller and diffuser, and tapered impeller designs were proposed and experiments were performed. Uneven pitch design of the impeller changes the sound quality while the overall sound power level (SPL) and the performance remains similar. The effect of the tapered design of impeller was evaluated. The trailing edge of the tapered fan is inclined. This reduces the flow interaction between the rotating impeller and the stationary diffuser because of some phase shifts. The static efficiency of the new impeller design is slightly lower than the previous design. However, the overall SPL is reduced by about 4 dB(A). The SPL of the fundamental blade passing frequency (BPF) is reduced by about 6 dB (A) and the 2$\^$nd/ BPF is reduced about 20 dB (A). The vacuum cleaner with the tapered impeller design produces lower noise level than the previous one, and the strong tonal sound was dramatically reduced.

• 한국음향학회지
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• 제23권8호
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• pp.583-589
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• 2004

포만트 등의 음향학적인 정보를 이용하지 않는 연속음성인식 (CSR)을 위한 벡터 양자화기 기반의 화자 정규화 방법을 제안한다. 이 방법은 앞서 제안한 간단한 숫자음 인식기를 위한 화자정규화 방법을 개선한 것으로, 코드북의 크기를 증가시켜 가면서 벡터양자화기를 반복적으로 학습시킴으로써 정규화된 코드북을 구한 다음, 치를 이용하여 시험용화자의 워핑계수를 추정한다. 코드북 생성과 워핑계수 추정을 위해 모음 음소의 집합과 자음과 모음을 포함한 모든 음소의 집합 등 두 가지 음소집합을 이용i,겨 실험하였으며, 추정한 워핑계수에 상응하는 구간선형 워핑함수를 이용하여 인식기의 학습과 시험에 사용될 특징벡터를 워핑하였다. TIMIT 코퍼스와 HTK toolkit을 이용한 음소인식 실험을 수행하여 제안하는 방법의 성능을 조사한 결과, 포만트를 이용한 워핑 방법과 비슷한 성능을 가짐을 확인하였다.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2012년도 춘계학술대회 논문집
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• pp.763-768
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• 2012

Active window system which can reduce the environmental noises, such as traffic noise and construction noise, from an open window into a room was proposed in the previous works. The key idea of the proposed active window system was that the control sources are approximately collocated with the primary noise source in terms of the acoustic power for global noise reduction throughout the interior room. Moreover, because it is important not to intrude into the living space in the building environment, no error sensors were used and an open-loop control method using control sources at the window frame and the reference sensors outside the room was used for the proposed system. The open-loop control gain was calculated by the interior room model assumed as the semi-infinite space, and the interior sound field was estimated by Rayleigh integral equation under the baffled window model assumption. However, windows with a finite thickness should were considered for the calculation of the open-loop control gain of the active window system since these are representative of most window cases. Therefore, the finite thickness window model based on the Sgard's model was derived and the open-loop control gain using the interior sound field estimated by that model was calculated for active window system. To compare the performance of these two models, a scale-model experiment was performed in an anechoic chamber according to noise source directions. Experimental results showed that the performance for the thickness window model is better than the baffled window model as the angle with respect to the perpendicular direction is larger.

• Ocean and Polar Research
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• 제36권2호
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• pp.103-110
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• 2014

A wind-driven current in the East Sea from Lagrangian measurements of wind and current at 15 m using MiniMet drifters was analyzed. Spectral analysis of the current from 217 pieces of a 10 day-long time series shows the dominant energy at the inertial frequency for the current at 15 m. Wind has energy peaks at a 0.2-0.5 cycles per day (cpd) frequency band. The power spectrum of the clockwise rotating component is predominant for the current and was 1.5-2 times larger than the anticlockwise rotating component for wind. Co-spectra between the wind and current show two peak frequency bands at subinertial frequency and 0.5-0.3 cpd. Coherences between the wind and current at those peak frequencies are significant with 95% confidence and phase differences were $90-100^{\circ}$. From the phase differences, the efolding depth is estimated as 17 m and this e-folding depth is smaller than the estimation by Chereskin's (1999) 25 m using a moored Acoustic Doppler Current Profiler and an anemometer installed at the surface buoy. The angle between the wind-driven current (or ageostrophic current) and wind from this study was also much larger than the global estimate by Rio and Hernandez (2003) using reanalysis wind and drifters. The possible explanation for the discrepancy comes from the fact that the current is driven by a wind of smaller length scale than 250 km but the satellite or the reanalysis products do not resolve winds of length scale smaller than 250 km. Large rms differences between Mini-Met and QuickSCAT wind on spatial lags smaller than 175 km substantiate this explanation.