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2018 IEEE Global Conference on Signal and Information Processing (GlobalSIP)最新文献

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STATISTICAL DETECTION AND CLASSIFICATION OF TRANSIENT SIGNALS IN LOW-BIT SAMPLING TIME-DOMAIN SIGNALS 低位采样时域信号中暂态信号的统计检测与分类
Pub Date : 2018-11-01 DOI: 10.1109/GLOBALSIP.2018.8646395
G. Nita, A. Keimpema, Z. Paragi
We investigate the performance of the generalized Spectral Kurtosis (SK) estimator in detecting and discriminating natural and artificial very short duration transients in the 2-bit sampling time domain Very-Long-Baseline Interferometry (VLBI) data. We demonstrate that, after a 32-bit FFT operation is performed on the 2-bit time domain voltages, these two types of transients become distinguishable from each other in the spectral domain. Thus, we demonstrate the ability of the Spectral Kurtosis estimator to automatically detect bright astronomical transient signals of interests - such as pulsar or fast radio bursts (FRB) - in VLBI data streams that have been severely contaminated by unwanted radio frequency interference.
本文研究了广义谱峰度(SK)估计在2位采样时域甚长基线干涉测量(VLBI)数据中检测和区分自然和人工极短持续时间瞬态的性能。我们证明,在对2位时域电压执行32位FFT操作后,这两种类型的瞬态在谱域中变得彼此可区分。因此,我们证明了谱峰度估计器在VLBI数据流中自动检测感兴趣的明亮天文瞬态信号(如脉冲星或快速射电暴(FRB))的能力,这些数据流已被不必要的射频干扰严重污染。
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引用次数: 1
EFFICIENT RFI DETECTION IN RADIO ASTRONOMY BASED ON COMPRESSIVE STATISTICAL SENSING 基于压缩统计感知的射电天文学rfi检测方法
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646517
G. Cucho‐Padin, Yue Wang, L. Waldrop, Z. Tian, F. Kamalabadi
In this paper, we present an efficient method for radio frequency interference (RFI) detection based on cyclic spectrum analysis that relies on compressive statistical sensing to estimate the cyclic spectrum from sub-Nyquist data. We refer to this method as compressive statistical sensing (CSS), since we utilize the statistical autocovariance matrix from the compressed data. We demonstrate the performance of this algorithm by analyzing radio astronomy data acquired from the Arecibo Observatory (AO)’s L-Wide band receiver (~1.3 GHz), which is typically corrupted by active radars for commercial applications located near AO facilities. Our CSS-based solution enables robust and efficient detection of the RFI frequency bands present in the data, which is measured by receiver operating characteristic (ROC) curves. As a result, it allows fast and computationally efficient identification of RFI-free frequency regions in wideband radio astronomy observations.
本文提出了一种基于循环频谱分析的射频干扰检测方法,该方法依靠压缩统计感知从亚奈奎斯特数据中估计循环频谱。我们将这种方法称为压缩统计感知(CSS),因为我们利用压缩数据中的统计自协方差矩阵。我们通过分析从阿雷西博天文台(AO)的l波段接收机(~1.3 GHz)获得的射电天文数据来证明该算法的性能,该接收机通常被位于AO设施附近的商业应用的有源雷达破坏。我们基于css的解决方案能够稳健有效地检测数据中存在的RFI频段,这是通过接收器工作特性(ROC)曲线测量的。因此,它允许在宽带射电天文观测中快速和计算高效地识别无射频信号的频率区域。
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引用次数: 1
Enhanced Indoor Navigation System with Beacons and Kalman Filters 带有信标和卡尔曼滤波器的增强室内导航系统
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646581
Andrew Mackey, P. Spachos, K. Plataniotis
Indoor positioning systems are used in a variety of applications from shopping malls and museums to subject monitoring and tracking. The reliability and usability of such systems are highly based on their accuracy as well as cost and ease of deployment. Although the Global Positioning System (GPS) is an accurate solution for outdoor use, it can not be used indoors. A popular approach is a wireless navigation system which makes use of Received Signal Strength Indicators (RSSI). However, signal propagation, as well as surrounding noise and a dynamic environment, can affect their performance. Recent advancements in Bluetooth Low Energy (BLE) devices and the introduction of small and inexpensive beacons can alleviate the problem. In this work, we introduce an indoor navigation system with BLE beacons. To measure system accuracy an Android application was developed to collect the signal. Moreover, a Kalman filter was also developed within the application to improve the accuracy. Experimental results showed improvement of systems accuracy in three square topologies. The Kalman filter improved the accuracy up to 78.9%. while the experiments also show a correlation between the overall accuracy and how close BLE beacons are to each other.
室内定位系统用于从购物中心和博物馆到主题监控和跟踪的各种应用。这些系统的可靠性和可用性在很大程度上取决于它们的准确性以及成本和部署的便利性。虽然全球定位系统(GPS)是户外使用的精确解决方案,但它不能在室内使用。一种流行的方法是利用接收信号强度指标(RSSI)的无线导航系统。然而,信号传播、周围噪声和动态环境都会影响它们的性能。蓝牙低功耗(BLE)设备的最新进展和小型廉价信标的引入可以缓解这个问题。本文介绍了一种基于BLE信标的室内导航系统。为了测量系统的精度,开发了一个Android应用程序来收集信号。此外,在应用程序中还开发了卡尔曼滤波器以提高精度。实验结果表明,在三种方形拓扑结构下,系统精度得到了提高。卡尔曼滤波将准确率提高到78.9%。而实验也显示了总体精度与BLE信标之间的距离之间的相关性。
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引用次数: 11
Nonlinear Dimensionality Reduction Via Polynomial Principal Component Analysis 基于多项式主成分分析的非线性降维
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646515
A. Kazemipour, S. Druckmann
In this paper, we introduce Poly-PCA, a nonlinear dimensionality reduction technique which can capture arbitrary nonlinearities in high-dimensional and dynamic data. Instead of optimizing over the space of nonlinear functions of high-dimensional data Poly-PCA models the data as nonlinear functions in the latent variables, leading to relatively fast optimization. Poly-PCA can handle nonlinearities which do not preserve the topology and geometry of the latents. Applying Poly-PCA to a nonlinear dynamical system successfully recovered the phase-space of the latent variables.
本文介绍了一种非线性降维技术Poly-PCA,它可以捕获高维动态数据中的任意非线性。Poly-PCA不是在高维数据的非线性函数空间上进行优化,而是将数据作为潜在变量中的非线性函数建模,从而实现相对快速的优化。Poly-PCA可以处理不保留电位拓扑和几何形状的非线性。将多元主成分分析应用于非线性动力系统,成功地恢复了潜在变量的相空间。
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引用次数: 0
l0-NORM FEATURE LMS ALGORITHMS 10范数特征LMS算法
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646465
Hamed Yazdanpanah, J. A. Apolinário, P. Diniz, Markus V. S. Lima
A class of algorithms known as feature least-mean-square (F-LMS) has been proposed recently to exploit hidden sparsity in adaptive filter parameters. In contrast to common sparsity-aware adaptive filtering algorithms, the F-LMS algorithm detects and exploits sparsity in linear combinations of filter coefficients. Indeed, by applying a feature matrix to the adaptive filter coefficients vector, the F-LMS algorithm can reveal and exploit their hidden sparsity. However, in many cases the unknown plant to be identified contains not only hidden but also plain sparsity and the F-LMS algorithm is unable to exploit it. Therefore, we can incorporate sparsity-promoting techniques into the F-LMS algorithm in order to allow the exploitation of plain sparsity. In this paper, by utilizing the l0-norm, we propose the l0-norm F-LMS (l0-F-LMS) algorithm for sparse lowpass and sparse highpass systems. Numerical results show that the proposed algorithm outperforms the F-LMS algorithm when dealing with hidden sparsity, particularly in highly sparse systems where the convergence rate is sped up significantly.
为了利用自适应滤波器参数的隐稀疏性,最近提出了一种称为特征最小均方(F-LMS)的算法。与常见的稀疏性感知自适应滤波算法相比,F-LMS算法检测并利用滤波系数线性组合中的稀疏性。事实上,通过将特征矩阵应用于自适应滤波器系数向量,F-LMS算法可以揭示和利用其隐藏的稀疏性。然而,在许多情况下,待识别的未知植物不仅包含隐藏的稀疏性,而且包含明显的稀疏性,而F-LMS算法无法利用它。因此,我们可以将促进稀疏性的技术合并到F-LMS算法中,以便允许利用纯稀疏性。本文利用10范数,提出了稀疏低通和稀疏高通系统的10范数F-LMS (10 -F-LMS)算法。数值结果表明,该算法在处理隐稀疏性时优于F-LMS算法,特别是在高度稀疏系统中,收敛速度明显加快。
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引用次数: 16
COINCIDENT PEAK PREDICTION USING A FEED-FORWARD NEURAL NETWORK 基于前馈神经网络的重合峰预测
Pub Date : 2018-11-01 DOI: 10.1109/GLOBALSIP.2018.8646654
Chase P. Dowling, D. Kirschen, Baosen Zhang
A significant portion of a business’ annual electrical payments can be made up of coincident peak charges: a transmission surcharge for power consumed when the entire system is at peak demand. This charge occurs only a few times annually, but with per-MW prices orders of magnitudes higher than non-peak times. A business is incentivized to reduce its power consumption, but accurately predicting the timing of peak demand charges is nontrivial. In this paper we present a decision framework based on predicting the day-ahead likelihood of peak demand charges. We train a feed-forward neural net-work to estimate the probability of system demand peaks and show it outperforms conventional forecasting methods using historical load. Using ERCOT demand and weather data from 2010-2017, we show the effectiveness of our framework.
企业年度电费的很大一部分可以由同步峰值费用组成:当整个系统处于需求峰值时消耗的电力的传输附加费。这种收费每年只发生几次,但每兆瓦的价格比非高峰时期高几个数量级。企业被激励去减少其电力消耗,但是准确预测高峰需求收费的时间是非常重要的。在本文中,我们提出了一个基于预测一天前高峰需求收费可能性的决策框架。我们训练了一个前馈神经网络来估计系统需求峰值的概率,并表明它优于传统的使用历史负荷的预测方法。利用2010-2017年的ERCOT需求和天气数据,我们展示了我们框架的有效性。
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引用次数: 3
Hybrid Wireless Localization via Complex-domain Isometric Embedding 基于复域等距嵌入的混合无线定位
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646519
G. Abreu, Alireza Ghods
We revisit the super multidimensional scaling (SMDS) wireless localization algorithm first proposed a decade ago, recasting it onto the complex-domain1. Under this new formulation, the edge kernel which carries both angle and distance information simultaneously and plays a central role in the SMDS algorithm, becomes a complex-valued rank-one matrix, resulting in a new complex-domain SMDS framework which yields several advantages over the original, including the elimination of redundancy and the enhancement of conditions to handle information erasure.
我们回顾了十年前首次提出的超多维缩放(SMDS)无线定位算法,并将其重新映射到complex-domain1上。在此框架下,在SMDS算法中起核心作用的同时携带角度和距离信息的边缘核变成复值秩一矩阵,从而形成了一种新的复杂域SMDS框架,该框架具有消除冗余和增强处理信息擦除条件等优点。
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引用次数: 0
OPTIMAL DATA TASK DISTRIBUTION FOR BALANCING ENERGY CONSUMPTION ON COOPERATIVE FOG NETWORKS 协同雾网络能耗平衡的数据任务优化分配
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646641
José Clemente, Fangyu Li, Wenzhan Song
In this paper, the problem of how to balance the energy consumption during data processing in networks is investigated using a fog middleware. We first demonstrate that for a fog network with different kind of nodes, balancing the energy relies on a combinatorial optimization that is solved using graph theory. We propose a transformation of the transshipment graph problem to formulate an optimization problem that we solve with linear programming (LP). We show the possibility of balancing and extending the battery life of the whole network based on cooperation between nodes without jeopardizing individual nodes’ battery life. We use both, emulation and real scenarios to test our optimization algorithm. We show we can balance the network energy, keep all nodes alive and active ~95% of the time.
本文利用雾中间件研究了网络中数据处理过程中能量消耗的平衡问题。我们首先证明,对于具有不同类型节点的雾网络,能量平衡依赖于使用图论解决的组合优化。本文提出了转运图问题的一个变换,以形成一个用线性规划求解的优化问题。我们展示了在不损害单个节点电池寿命的情况下,基于节点之间的合作来平衡和延长整个网络电池寿命的可能性。我们使用仿真和真实场景来测试我们的优化算法。我们证明我们可以平衡网络能量,使所有节点在95%的时间内保持活跃。
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引用次数: 2
DIFFERENTIALLY PRIVATE SPARSE INVERSE COVARIANCE ESTIMATION 差分私有稀疏逆协方差估计
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646444
Di Wang, Mengdi Huai, Jinhui Xu
In this paper, we present the first results on the sparse inverse covariance estimation problem under the differential privacy model. We first gave an ε-differentially private algorithm using output perturbation strategy, which is based on the sensitivity of the optimization problem and the Wishart mechanism. To further improve this result, we then introduce a general covariance perturbation method to achieve both ε-differential privacy and (ε, δ)-differential privacy. For ε-differential privacy, we analyze the performance of Laplacian and Wishart mechanisms, and for (ε, δ)-differential privacy, we examine the performance of Gaussian and Wishart mechanisms. Experiments on both synthetic and benchmark datasets confirm our theoretical analysis.
本文给出了差分隐私模型下稀疏反协方差估计问题的初步结果。首先基于优化问题的敏感性和Wishart机制,提出了一种基于输出摄动策略的ε-差分私有算法。为了进一步改进这一结果,我们引入了一种通用的协方差摄动方法来实现ε-微分隐私和(ε, δ)-微分隐私。对于ε-微分隐私,我们分析了拉普拉斯机制和Wishart机制的性能,对于(ε, δ)-微分隐私,我们研究了高斯机制和Wishart机制的性能。在合成数据集和基准数据集上的实验证实了我们的理论分析。
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引用次数: 8
SPATIAL FOURIER TRANSFORM FOR DETECTION AND ANALYSIS OF PERIODIC ASTROPHYSICAL PULSES 空间傅里叶变换用于周期性天体物理脉冲的探测和分析
Pub Date : 2018-11-01 DOI: 10.1109/GlobalSIP.2018.8646706
Marwan Alkhweldi, N. Schmid
This paper analyzes the potential of the Spatial Fourier transform (SFT) for detection of a periodic astrophysical signal and for estimation of parameters of the signal. In place of de-dispersing filter bank data for each Dispersion Measure (DM) trial and then integrating over frequency channels to yield a one-dimensional signal, we apply SFT to filter bank data, then detect periodic astrophysical signals and analyze their parameters such as DM and rotational period. This approach allows searching for periodic astrophysical signals in real time. Its complexity is dominated by the complexity of the SFT. The results of our analysis show promise. Using simulated data we demonstrate that it takes about 3 minutes of observation time to detect a pulsar at an S/N value of 8σ. The SFT data also provide information about the rotation of pulsars and lower and upper bounds on their DM value.
本文分析了空间傅里叶变换(SFT)在周期性天体物理信号检测和信号参数估计方面的潜力。为了代替每次色散测量(DM)试验的去色散滤波组数据,然后在频率通道上进行积分以产生一维信号,我们应用SFT对组数据进行滤波,然后检测周期性天体物理信号并分析其参数,如DM和旋转周期。这种方法可以实时搜索周期性的天体物理信号。它的复杂性主要取决于SFT的复杂性。我们的分析结果显示出了希望。利用模拟数据表明,探测到信噪比为8σ的脉冲星大约需要3分钟的观测时间。SFT数据还提供了脉冲星的旋转和它们的DM值的上下边界的信息。
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引用次数: 0
期刊
2018 IEEE Global Conference on Signal and Information Processing (GlobalSIP)
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