• 한국실내디자인학회논문집
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• 제18권1호
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• pp.64-71
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• 2009

The modern society is rapidly changing through the development of computer network technology. By generation a collapse of boundaries between may important social institutions, computer networking has affected culture, economy and the physical environment. Because of this, people face a switchover from a simple society, to a compound society. It will also increase the diversity if society's demand, though, and experience. This change is not an exception in the exhibition space. People are more interested in civilized pastimes and also demand diverse thinking. So as a necessary consequence, the function of museum space Is offended and that there are various attempt to increase information and demand of that space. The purpose of this study is try to find a solution a countermeasure of modern society's mobile situation. Researchers analyzed structural qualities of Hyper-text; non-boundary, interaction and nonlinear and deduce nine kinds of methods to apply in space. Also, Researchers looked at the examples in museum space and derived like this expression way; dynamics, mobility, a non-materiality, continuity, complexity from analysis of expression way.

• 한국해양공학회지
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• 제20권2호
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• pp.16-21
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• 2006

This paper discusses the behavior of post-tensioned and shaped hypar space truss, with consideration of the influence of removing some web members. Hypar space truss is post-tensioned at the bottom chords of one diagonal on the ground; the essential behavior characteristic of shape formation is discussed by using a small-scale test model. Results of experiments and nonlinear finite-element analysis indicate that a planar, rectangular- arranged structure can be deformed to a predicted hyper shape, by the proposed shape formation method. Also the feasibility of the proposed method for furnishing of a hypar shaped face truss has been presented, under the condition of both non-removed and partially removed web members. It follows that a nonlinear finite element analysis method can be used in predicting the behavior of the space shape and the post-tensioning force in sharing of hypar space truss. Further, in comparison to the other cases, the results of test and analysis show that the active diagonal shaping in the non-removed web members and passive diagonal shaping of partially removed web members are in relatively good agreement.

• 방송공학회논문지
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• 제28권2호
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• pp.213-229
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• 2023

본 논문에서는 가상환경에 위치한 청취자의 움직임에 대응하여 실시간으로 6DoF 공간음향을 제공하는 공간음향 렌더링 시스템에 대해 소개한다. 본 시스템은 MPEG-I Immersive Audio CfP 대응을 위하여 MPEG-I AEP를 개발환경으로 사용하여 구현되었으며 인코더와, 디코더를 포함하는 렌더러로 구성된다. 인코더는 인코더 입력 포맷(EIF) 파일에 포함된 가상공간 장면의 공간적 오디오 파라미터와, SOFA 파일로 제공되는 음원의 지향성 정보 등의 메타데이터를 오프라인으로 부호화하여 비트스트림으로 전달하는 역할을 하며, 렌더러는 전달된 비트스트림을 수신하여 청취자의 위치에 따라 실시간으로 6DoF 공간음향 렌더링을 수행한다. 개발된 렌더링 시스템에 적용한 주요 공간음향 처리 기술로는 음원 효과 및 장애물 효과 처리 기술이 있으며, 그 외 시스템 동작에 필요한 기술로는 도플러 효과 및 음장효과 처리 기술 등이 있다. 개발된 시스템에 대한 성능평가 결과로서 자체 주관평가 결과를 소개한다.

• 천문학논총
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• 제32권1호
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• pp.225-230
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• 2017

The extragalactic background suggests half the energy generated by stars was reprocessed into the infrared (IR) by dust. At z~1.3, 90% of star formation is obscured by dust. To fully understand the cosmic star formation history, it is critical to investigate infrared emission. AKARI has made deep mid-IR observation using its continuous 9-band filters in the NEP field ($5.4deg^2$), using ~10% of the entire pointed observations available throughout its lifetime. However, there remain 11,000 AKARI infrared sources undetected with the previous CFHT/Megacam imaging (r ~25.9ABmag). Redshift and IR luminosity of these sources are unknown. These sources may contribute significantly to the cosmic star-formation rate density (CSFRD). For example, if they all lie at 1< z <2, the CSFRD will be twice as high at the epoch. We are carrying out deep imaging of the NEP field in 5 broad bands (g, r, i, z, and y) using Hyper Suprime-Camera (HSC), which has 1.5 deg field of view in diameter on Subaru 8m telescope. This will provide photometric redshift information, and thereby IR luminosity for the previously-undetected 11,000 faint AKARI IR sources. Combined with AKARI's mid-IR AGN/SF diagnosis, and accurate midIR luminosity measurement, this will allow a complete census of cosmic star-formation/AGN accretion history obscured by dust.

• 대기
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• 제19권4호
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• pp.319-329
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• 2009

The intensive dust observation experiment has been performed at Korea Global Atmosphere Watch Center (KGAW) in Anmyeon, Korea during each spring season from 2007 to 2009. Downward and upward hyper-spectral spectrums over the dust condition were measured to understand the hyper-spectral properties of Asian dust using both ground-based Fourier Transform Infrared Spectroscopy (FT-IR) and space-borne AIRS/Aqua. To understand the impact of the Asian dust, a Line-by-Line radiative transfer model runs to calculate the high resolution infrared spectrum over the wave number range of $500-500cm^{-1}$. Furthermore, the radiosonde, a $PM_{10}$ Sampler, a Micro Pulse Lidar (MPL), and an Aerodynamic Particle Sizer (APS) are used to understand the vertical profile of temperature and humidity and the properties of Asian dust like concentration, altitude of dust layer, and size distribution. In this study, we found the Asian dust distributed from surface up to 3-4 km and volume concentration is increased at the size range between 2 and $8{\mu}m$ The observed dust spectrums are larger than the calculated clear sky spectrums by 15~60K for downward and lower by around 2~6K for upward in the wave number range of $800-1200cm^{-1}$. For the characteristics of the spectrum during the Asian dust, the downward spectrum is revealed a positive slope for $800-1000cm^{-1}$ region and negative slope over $1100-1200cm^{-1}$ region. In the upward spectrum, slopes are opposed to the downward one. It is inferred that the difference between measured and calculated spectrum is mostly due to the contribution of emission and/or absorption of the dust particles by the aerosol amount, size distribution, altitude, and composition.

• 한국정보통신학회논문지
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• 제11권2호
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• pp.229-238
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• 2007

인터넷의 기술을 기반으로 사이버 공간에서 상업적인 목적의 새로운 비즈니스 형태인 사이버 쇼핑몰이 생겨났다. 사이버 쇼핑몰의 경제 활동은 과거 실물경제에 비해 상승폭이 매우 크며 앞으로도 더욱 성장할 것이다. 따라서, 본 논문에서는 상호작용형 인터넷 쇼핑몰을 제안한다. 특히 본 논문에서 제안하는 쇼핑몰은 기존의 쇼핑몰과는 달리 리치미디어 기술 기반의 상호작용형 3D 가상 쇼핑몰에 기초를 하고 있다. 이러한 시스템은 가상의 공간을 투어 하면서 추매하고자 하는 오브젝트를 클릭 하였을 때 그 오브젝트에 Hyper view의 형식으로 표현되며, 이는 기존 방식과는 달리 오브젝트를 이동, 회전, 확대, 축소 그리고, 실행까지도 가능하게 한다. 쇼핑의 형태가 소비자들에게 흥미감과 몰입감을 증대시킬 수 있고, 기존에 쇼핑몰이 가지고 있는 2D의 이미지 중심에서 탈피하여 3D의 모델링 제품을 통한 현실적인 제품의 표현은 구매의도 향상에 크게 기여 할 것이다.

• 융합보안논문지
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• 제22권1호
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• pp.129-134
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• 2022

스마트플랫폼이란 기존 플랫폼과 첨단 IT기술을 결합함으로써 물리 및 가상공간을 초연결 환경으로 구현한 진화된 플랫폼이라 정의된다. 초연결로 언급되는 정보와 정보, 인프라와 인프라, 인프라와 정보, 공간과 서비스가 연결은 사용자의 삶의 질과 환경을 획기적으로 변화시켜 주는 고품질의 서비스 구현 및 제공을 가능하게 한다. 특히 스마트 정부와 스마트 헬스케어 구현으로 사회안전망과 개인건강관리 수준을 획기적으로 개선시킨 효과를 모두에게 제공하고 있다. 이 과정에서 생산되고 소비되는 수많은 정보들은 그 자체로서 혹은 빅데이터 분석을 통해 공공 및 개인의 기본권을 위협하는 요인으로 작용할 수 있다. 특히 스마트시티의 생태계를 형성하는 핵심기능으로서의 스마트플랫폼은 자연스럽게 지속적으로 확장되어 가기 때문에 그에 따르는 데이터의 처리운용과 네트워크 운영 상 커다란 보안 부담에 직면하고 있다. 이 논문에서는 스마트시티의 핵심 기능으로서의 플랫폼 구성 요소와 그에 대한 적절한 보안위협 및 대응 방안을 연구한다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.37.2-37.2
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• 2008

Korea-Japan Joint VLBI Correlator (KJJVC), to be used for Korean VLBI Network (KVN) in Korea Astronomy & Space Science Institute (KASI), is a high-speed calculator that outputs the correlation results in the maximum speed of 1.4GB/sec.To receive and record this data keeping up with this speed and with no loss, the design of the software running on the data archive system for receving and recording the output data from the correlator is very important. But, the simple kind of programming using just single thread that receives data from network and records it by turns, can cause a bottleneck effect while processing high speed data and a probable data loss, and cannot utilize the merit of hardwares supporting multi core or hyper threading, or operating systems supporting these hardwares. In this talk we summarize the design of the data transfer software for KJJVC and high speed, large capacity data archive system using general socket programming and multi threading techniques, and the pre-BMT(Bench Marking Test) results from the tests of the storage product providers' proposals using this software.

• International Journal of Aeronautical and Space Sciences
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• 제18권2호
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• pp.175-185
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• 2017

This paper presents new differential methods for computing the combined and single dynamic stability derivatives of flight vehicle. Based on rigid dynamic mesh technique, the combined dynamic stability derivative can be achieved by imposing the aircraft pitching to the same angle of attack with two different pitching angular velocities and also translating it to the same additional angle of attack with two different rates of angle of attack. As a result, the acceleration derivative is identified. Moreover, the rotating reference frame is adopted to calculate the rotary derivatives when simulating the steady pull-up with different pitching angular velocities. Two configurations, the Hyper Ballistic Shape (HBS) and Finner missile model, are considered as evaluations and results of all the cases agree well with reference or experiment data. Compared to traditional ones, the new differential methods are of high efficiency and accuracy, and potential to be extended to the simulation of combined and single stability derivatives of directional and lateral.

• 천문학회지
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• 제34권4호
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• pp.321-323
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• 2001

Compressible, magnetohydrodynamic (MHD) turbulence in two dimension is studied through high-resolution, numerical simulations with the isothermal equation of state. First, hydrodynamic turbulence with Mach number $(M)_{rms}\;\~$1 is generated by enforcing a random force. Next, initial, uniform magnetic field of various strengths with Alfvenic Mach number Ma $\gg$ 1 is added. Then, the simulations are followed until MHD turbulence is fully developed. Such turbulence is expected to exist in a variety of astrophysical environments including clusters of galaxies. Although no dissipation is included explicitly in our simulations, truncation errors produce dissipation which induces numerical resistivity. It mimics a hyper-resistivity in our second-order accurate code. After saturation, the resulting flows are categorized as SF (strong field), WF (weak field), and VWF (very weak field) classes respectively, depending on the average magnetic field strength described with Alfvenic Mach number, $(Ma)_{rms}{\ge}1$, $(Ma)_{rms}{\~}1$, and $(Ma)_{rms}{\gg}1$. The characteristics of each class are discussed.