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An Efficient Soft-Output MIMO Detection Method Based on a Multiple-Channel-Ordering Technique
임태호,박인수,유현종,유성욱,조용수 한국전자통신연구원 2011 ETRI Journal Vol.33 No.5
In this paper, we propose an efficient soft-output signal detection method for spatially multiplexed multiple-input multiple-output (MIMO) systems. The proposed method is based on the ordered successive interference cancellation (OSIC) algorithm, but it significantly improves the performance of the original OSIC algorithm by solving the error propagation problem. The proposed method combines this enhanced OSIC algorithm with a multiple-channel-ordering technique in a very efficient way. As a result, the log likelihood ratio values can be computed by using a very small set of candidate symbol vectors. The proposed method has been synthesized with a 0.13-μm CMOS technology for a 4x4 16-QAM MIMO system. The simulation and implementation results show that the proposed detector provides a very good solution in terms of performance and hardware complexity.
임태호,김재권,조용수,Im, Tae-Ho,Kim, Jae-Gwon,Cho, Yong-Su 한국통신학회 2007 정보와 통신 Vol.24 No.8
다중안테나 시스템은 단일 안테나 시스템에 비해 추가적인 주파수나 송신전력의 할당 없이 채널 용량을 안테나 수에 비례하여 증가시킬 수 있다는 장점으로 인해 차세대 통신기술의 핵심으로 부각되고 있다. 본 고에서는 이와 같은 장점을 가지고 있는 다중안테나 시스템의 신호검출을 위한 다양한 기법을 기술한다. 특히 공간다중화 방식의 다중 송수신 안테나 시스템에서의 다양한 신호검출 기법을 살펴보고, 성능 및 연산복잡도면에서 비교한다.
Far-ultraviolet Observations of the Taurus-Perseus-Auriga Complex
임태호,민경욱,선광일,Lim, Tae-Ho,Min, Kyoung-Wook,Seon, Kwang-Il 한국천문학회 2012 天文學會報 Vol.37 No.2
We firstly present the unified Far-UV continuum map of the Taurus-Auriga-Perseus (TPA) complex, one of the largest local associations of dark cloud located in (l, b)=([154,180], [-28, -2]), by merging both FIMS and GALEX. The FUV continuum map shows that dust extinction correlate well with the FUV around the complex. It shows strong absorption in FUV toward the dense Taurus cloud while it does not in California cloud. It turned out that it is related to the relative location of each cloud and Perseus OB2 association. We also present some results of dust scattering simulation based on Monte Carlo Radiative Transfer technique (MCRT). Through this dust scattering simulation, we have derived the scattering parameter for this region, albedo(a)=$0.42^{+0.05}{_{-0.05}}$, asymmetry factor(g)=$0.47^{+0.11}{_{-0.27}}$. The optical parameters we obtained seem reasonable compared to the theoretical model values ~0.40 and ~0.65 for the albedo and the phase function though the phase function is rather small. Using the result of simulation, we figured out the geometries of each cloud in the complex region, especially their distances and thicknesses. Our predictions from the results are in good agreement with the previous studies related to the TPA complex. For example, the Taurus cloud is within ~200pc from the Sun and the Perseus seems to be multi-layered, at least two. The California cloud is more distant than the other cloud on average at ~350 pc and Auriga cloud seems to be between the Taurus cloud and the eastern end of the California cloud. We figured out that across the TPA complex region, there might be some correlation between the LSR velocity and the distance to each cloud in the complex.