• Proceedings of the Korean Society of Broadcast Engineers Conference
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• 2016.11a
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• pp.78-79
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• 2016

본 논문에서는 국내 지상파 UHDTV 송수신 정합 규격을 기반으로, 방송 송출 환경에 따라 기존 방송 채널과 더불어 특정 시간 동안에 별도의 서비스 채널 추가적으로 운용할 수 있는 동적 다채널 방송 서비스를 제안하고 서비스 운용 방법을 소개한다. 제안하는 동적 다채널 방송 서비스를 구성하는 가상 채널은 지상파 방송망뿐만 아니라 브로드밴드망으로도 구성될 수 있다. 또한 본 논문에서는 동적 다채널 방송 서비스 구간에서 지상파 방송망으로 전달되는 기존 채널과 브로드밴드망을 통해 동적으로 생성된 채널간의 유연한 채널 전환이 이뤄질 수 있도록 채널 연결성 정보를 구현하였으며, 이를 수신기에 전달하여 채널간의 끊김 없는 UHDTV 서비스 제공이 가능함을 확인하였다.

• The Journal of the Acoustical Society of Korea
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• v.20 no.1
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• pp.30-35
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• 2001

The most important characteristic of Emile Bell's sound is a beating. It is modulation phenomenon which appears as a result of interference multiplication in time domain. This modulation phenomenon can be modeled as DSB-SC which suppress carrier and signals distributed both sides. The beatiog wave is observed in Laman distribution signal for polyvinyl speech signal, water vein wave, tide wave. The beating wave is caused by asymmetry Property of the bell.

• Proceedings of the KIPE Conference
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• 2015.07a
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• pp.245-246
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• 2015

본 논문에서는 삼중 델타 전원과 새로운 커먼-모드 필터 결선을 통해 스위칭에 의한 고조파를 저감하는 방법을 제안한다. PWM에 의해 생성되는 측대파 고조파(Sideband harmonics) 위상을 분석함으로써, 인터리빙 운전 시 삼중 델타 전원 연결과 제안된 커먼모드 필터가 측대파 고조파 전류를 크게 저감할 수 있음을 보인다. 3개의 고정자 권선을 가지는 영구자석 전동기를 이용하여 제안된 필터의 유효성을 검증하였다.

• The Bulletin of The Korean Astronomical Society
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• v.46 no.2
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• pp.60.3-60.3
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• 2021

Squeezed vacuum injection을 이용한 중력파 검출기의 관측감도 향상 기술은 중력파 검출기 광신호의 양자 잡음을 제어하여 관측감도를 높이는 기술로 이론적으로는 10dB에 가까운 신호 대 잡음비 향상을 달성할 수 있다. 실험실 환경에서는 이미 10dB 이상의 신호 대 잡음비 향상을 달성했으며 실제 중력파 검출기에서는 GEO600의 6dB의 신호 대 잡음비 향상이 현재까지 가장 높은 수준이다. 한국천문연구원에서는 2019년부터 차세대 중력파 검출기 기술개발로 1064 nm 파장의 squeezer 개발을 추진했으며 현재 parametric down conversion을 이용해 squeezed vacuum을 생성하는 공진기를 제작하여 시험하는 단계에 있다. 이 발표에서는 한국천문연구원의 1064 nm squeezer 개발 연구와 개발 현황에 대해 소개하고자 한다.

• Journal of Broadcast Engineering
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• v.24 no.1
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• pp.118-131
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• 2019

In order to provide 8K UHD contents of terrestrial broadcasting with a large capacity, the terrestrial broadcasting system has various problems such as limited bandwidth and so on. To solve these problems, UHD contents transmission technology has been actively studied, and an 8K UHD broadcasting system using terrestrial broadcasting network and communication network has been proposed. The proposed technique is to solve the limited bandwidth problem of terrestrial broadcasting network by segmenting 8K UHD contents and transmitting them to heterogeneous networks through hierarchical separation. Through the terrestrial broadcasting network, the base layer corresponding to FHD and the additional enhancement layer data for 4K UHD are transmitted, and the additional enhancement layer data corresponding to 8K UHD is transmitted through the communication network. When 8K UHD contents are provided in such a way, user can receive up to 4K UHD broadcasting by terrestrial channels, and also can receive up to 8K UHD additional communication networks. However, in order to transmit the 4K UHD contents within the allocated bit rate of the domestic terrestrial UHD broadcasting, the compression rate is increased, so a certain level of image deterioration occurs inevitably. Due to the nature of UHD contents, video quality should be considered as a top priority over other factors, so that video quality should be guaranteed even within a limited bit rate. This requires packet scheduling of content generators in the broadcasting system. Since the multiplexer sends out the packets received from the content generator in order, it is very important to make the transmission time and the transmission rate of the process from the content generator to the multiplexer constant and accurate. Therefore, we propose a variable transmission scheduler between the content generator and the multiplexer to guarantee the image quality of a certain level of UHD contents in this paper.

• Geophysics and Geophysical Exploration
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• v.12 no.1
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• pp.85-98
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• 2009

The tau-p inversion algorithm is widely employed to generate starting models with most computer programs, which implement refraction tomography. This algorithm emphasises the vertical resolution of many layers, and as a result, it frequently fails to detect even large lateral variations in seismic velocities, such as the decreases which are indicative of shear zones. This study demonstrates the failure of the tau-p inversion algorithm to detect or define a major shear zone which is 50m or 10 stations wide. Furthermore, the majority of refraction tomography programs parameterise the seismic velocities within each layer with vertical velocity gradients. By contrast, the Generalized Reciprocal Method (GRM) inversion algorithms emphasise the lateral resolution of individual layers. This study demonstrates the successful detection and definition of the 50m wide shear zone with the GRM inversion algorithms. The existence of the shear zone is confirmed by a 2D analysis of the head wave amplitudes and by numerous closely spaced orthogonal seismic profiles carried out as part of a later 3D refraction investigation. Furthermore, an analysis of the shot record amplitudes indicates that a reversal in the seismic velocities, rather than vertical velocity gradients, occurs in the weathered layers. The major conclusion reached in this study is that while all seismic refraction operations should aim to provide as accurate depth estimates as is practical, those which emphasise the lateral resolution of individual layers generate more useful results for geotechnical and environmental applications. The advantages of the improved lateral resolution are obtained with 2D traverses in which the structural features can be recognised from the magnitudes of the variations in the seismic velocities. Furthermore, the spatial patterns obtained with 3D investigations facilitate the recognition of structural features such as faults which do not display any intrinsic variation or 'signature' in seismic velocities.

• Journal of the Korean Society of Marine Environment & Safety
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• v.21 no.2
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• pp.215-222
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• 2015

To improve the ocean waves of the ship maneuvering simulator, we study and summarize the visualization elements of the ocean waves and the overall direction of their implementation in detail. We categorize the visualization elements of the ocean waves into five groups, including wave surface, wave breaking, interaction, lighting effects, and underwater. We also analyze the design and implementation issues of the visualization of the ocean waves for ship maneuvering simulator with respect to realistic and real-time ocean visualization, ship dynamics, and application purposes. Through the analysis, we have found that the realistic visualization of ocean waves plays an important role in the generation of immersiveness, more accurate ship motion, and the various and controllable simulation scenarios for the ship maneuvering simulator. Additionally, we have confirmed that there are many visualization elements, methods, and limitations to be considered for the visualization of the ocean waves for ship maneuvering simulator, and we have concluded that the systematic design is required before implementation.

• Proceedings of the Korean Society of Propulsion Engineers Conference
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• 2011.11a
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• pp.263-267
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• 2011

This paper presents a numerical investigation of the deflagration to detonation transition (DDT) of flame acceleration by a shock wave filled with an ethylene-air mixture in bent tube. A model consisting of the reactive compressible Navier-Stokes equations and the ghost fluid method (GFM) for complex boundary treatment is used. A various intensities of incident shock wave simulations show the generation of hot spots by shock-flame interaction and the accelerated flame propagation due to geometrical effect. Also the first detonation occurs nearly constant chemical heat release rate, 20 MJ/($g{\cdot}s$). Through our simulation's results, we concentrate the complex confinement effects in generating strong shock wave, shock-flame interaction, hot spot and DDT in pipe.

• Journal of Astronomy and Space Sciences
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• v.25 no.1
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• pp.25-32
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• 2008

Using the solar wind data of 2000 observed by ACE, We classified the interplanetary shock on basis of shock driver. We examined the physical properties of shock drivers such as the ratio of charge states(O7/O6) and thermal index$(I_{th})$. Most of 51 interplanetary shocks are driven by interplanetary coronal mass ejections(ICME; magnetic cloud and ejecta) and high speed streams. According to the test of temperature(O7/O6) and $I_{th}$, we found that ICMEs originated from region with hot source in corona.

• Proceedings of the KIPE Conference
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• 2014.07a
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• pp.227-228
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• 2014

열차가 주행하는 선로에 설치되는 궤도회로는 레일 자체를 전기회로의 일부로 사용하여 일정 구간 내의 차량 유무를 판단하기 위한 회로이다. 국내의 경우 사용 주파수에 따라 전원전압 주파수의 짝수 고조파 대역을 사용하는 고속선 궤도회로와 홀수 고조파 대역을 이용하는 일반선 궤도회로로 구분할 수 있다. 이러한 궤도회로가 설치된 선로를 주행하는 고속차량의 주전력변환장치 컨버터는 단위 역률 제어를 수행하기 위하여 전원전압의 홀수 배수의 스위칭 주파수를 가지고 있기 때문에 컨버터 동작 시 가선전류에 고조파 전류가 생성된다. 이 때 컨버터부에서 발생되는 고조파 전류의 주파수와 궤도회로의 사용 주파수 대역이 일치하는 경우에 궤도회로의 오작동을 유발할 수 있다. 본 논문에서는 입력 컨버터부에서 사용하는 스위칭 주파수를 운행 구간에 따라 가변시켜 궤도회로 간섭 고조파 성분을 제어하는 방법을 제안하고 시험을 통해 성능을 확인하였다.