• Journal of Positioning, Navigation, and Timing
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• 제8권4호
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• pp.193-200
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• 2019

The auto-encoder network which is a good candidate to handle the modeling of the signal strength attenuation is designed for denoising and compensating the distortion of the received data. It provides a non-linear mapping function by iteratively learning the encoder and the decoder. The encoder is the non-linear mapping function, and the decoder demands accurate data reconstruction from the representation generated by the encoder. In addition, the adaptive network width which supports the automatic generation of new hidden nodes and pruning of inconsequential nodes is also implemented in the proposed algorithm for increasing the efficiency of the algorithm. Simulation results show that the proposed method can improve the neural network training surface to achieve the highest possible accuracy of the signal modeling compared with the conventional modeling method.

• Journal of Astronomy and Space Sciences
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• 제29권2호
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• pp.151-161
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• 2012

An intensive analysis of 148 timings of V700 Cyg was performed, including our new timings and 59 timings calculated from the super wide angle search for planets (SWASP) observations, and the dynamical evidence of the W UMa W subtype binary was examined. It was found that the orbital period of the system has varied over approximately $66^y$ in two complicated cyclical components superposed on a weak upward parabolic path. The orbital period secularly increased at a rate of $+8.7({\pm}3.4){\times}10^{-9}$ day/year, which is one order of magnitude lower than those obtained by previous investigators. The small secular period increase is interpreted as a combination of both angular momentum loss (due to magnetic braking) and mass-transfer from the less massive component to the more massive component. One cyclical component had a $20.^y3$ period with an amplitude of $0.^d0037$, and the other had a $62.^y8$ period with an amplitude of $0.^d0258$. The components had an approximate 1:3 relation between their periods and a 1:7 ratio between their amplitudes. Two plausible mechanisms (i.e., the light-time effects [LTEs] caused by the presence of additional bodies and the Applegate model) were considered as possible explanations for the cyclical components. Based on the LTE interpretation, the minimum masses of 0.29 $M_{\odot}$ for the shorter period and 0.50 $M_{\odot}$ for the longer one were calculated. The total light contributions were within 5%, which was in agreement with the 3% third-light obtained from the light curve synthesis performed by Yang & Dai (2009). The Applegate model parameters show that the root mean square luminosity variations (relative to the luminosities of the eclipsing components) are 3 times smaller than the nominal value (${\Delta}L/L_{p,s}{\approx}0.1$), indicating that the variations are hardly detectable from the light curves. Presently, the LTE interpretation (due to the third and fourth stars) is preferred as the possible cause of the two cycling period changes. A possible evolutionary implication for the V700 Cyg system is discussed.

• 전자공학회논문지
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• 제53권9호
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• pp.18-25
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• 2016

셀룰러 네트워크 환경에서 단말 간 직접통신(D2D : Device-to-Device)을 위해서는 기존의 셀룰러 링크의 성능을 보장함과 동시에 D2D 통신 링크의 성능을 극대화하는 것이 중요하다. 따라서 D2D 통신에 사용할 자원을 할당함에 있어 D2D 송신 단말이 셀룰러 시스템에 미치는 간섭과 셀룰러 시스템이 D2D 수신 단말에 주는 간섭을 동시에 고려해야 한다. 본 논문에서는 D2D 송신기와 수신기로 이루어진 D2D 링크가 셀룰러 시스템의 상향링크 자원을 공유하는 상황에서 복수의 D2D 링크에 효과적으로 자원을 할당하는 기법을 제안한다. 기지국은 인접 셀의 기지국과 정보 교환을 통해 셀 내의 단말들의 위치 정보를 공유한다는 가정 하에 단말들의 단말 위치 정보를 이용하여 D2D 링크와 셀룰러 링크 사이의 간섭을 최소화하는 자원을 할당한다. 아울러 경로손실 모델을 이용하여 계산한 셀룰러 링크 보호 상수 및 D2D 링크 보호 상수를 이용하여 셀룰러 링크와 D2D 링크 상호간의 간섭 및 D2D 링크 간의 간섭을 제한한다. 모의실험을 통해 제안한 자원할당 기법의 성능을 검증한다.