Time-Frequency Analysis of Radar Signals
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Moving Average Filters
CHAPTER 15 Moving Average Filters The moving average is the most common filter in DSP, mainly because it is the easiest digital filter to understand and use. In spite of its simplicity, the moving average filter is optimal for a common task: reducing random noise while retaining a sharp step response. This makes it the premier filter for time domain encoded signals. However, the moving average is the worst filter for frequency domain encoded signals, with little ability to separate one band of frequencies from another. Relatives of the moving average filter include the Gaussian, Blackman, and multiple- pass moving average. These have slightly better performance in the frequency domain, at the expense of increased computation time. Implementation by Convolution As the name implies, the moving average filter operates by averaging a number of points from the input signal to produce each point in the output signal. In equation form, this is written: EQUATION 15-1 Equation of the moving average filter. In M &1 this equation, x[ ] is the input signal, y[ ] is ' 1 % y[i] j x [i j ] the output signal, and M is the number of M j'0 points used in the moving average. This equation only uses points on one side of the output sample being calculated. Where x[ ] is the input signal, y[ ] is the output signal, and M is the number of points in the average. For example, in a 5 point moving average filter, point 80 in the output signal is given by: x [80] % x [81] % x [82] % x [83] % x [84] y [80] ' 5 277 278 The Scientist and Engineer's Guide to Digital Signal Processing As an alternative, the group of points from the input signal can be chosen symmetrically around the output point: x[78] % x[79] % x[80] % x[81] % x[82] y[80] ' 5 This corresponds to changing the summation in Eq. -
Power Grid Topology Classification Based on Time Domain Analysis
Power Grid Topology Classification Based on Time Domain Analysis Jia He, Maggie X. Cheng and Mariesa L. Crow, Fellow, IEEE Abstract—Power system monitoring is significantly im- all depend on the correct network topology information. proved with the use of Phasor Measurement Units (PMUs). Topology change, no matter what caused it, must be The availability of PMU data and recent advances in ma- immediately updated. An unattended topology error may chine learning together enable advanced data analysis that lead to cascading power outages and cause large scale is critical for real-time fault detection and diagnosis. This blackout ( [2], [3]). In this paper, we demonstrate that paper focuses on the problem of power line outage. We use a machine learning framework and consider the problem using a machine learning approach and real-time mea- of line outage identification as a classification problem in surement data we can timely and accurately identify the machine learning. The method is data-driven and does outage location. We leverage PMU data and consider not rely on the results of other analysis such as power the task of identifying the location of line outage as flow analysis and solving power system equations. Since it a classification problem. The methods can be applied does not involve using power system parameters to solve in real-time. Although training a classifier can be time- equations, it is applicable even when such parameters are consuming, the prediction of power line status can be unavailable. The proposed method uses only voltage phasor done in real-time. angles obtained from PMUs. -
Logistic-Weighted Regression Improves Decoding of Finger Flexion from Electrocorticographic Signals
Logistic-weighted Regression Improves Decoding of Finger Flexion from Electrocorticographic Signals Weixuan Chen*-IEEE Student Member, Xilin Liu-IEEE Student Member, and Brian Litt-IEEE Senior Member Abstract— One of the most interesting applications of brain linear Wiener filter [7–10]. To take into account the computer interfaces (BCIs) is movement prediction. With the physiological, physical, and mechanical constraints that development of invasive recording techniques and decoding affect the flexion of limbs, some studies applied switching algorithms in the past ten years, many single neuron-based and models [11] or Bayesian models [12,13] to the results of electrocorticography (ECoG)-based studies have been able to linear regressions above. Other studies have explored the decode trajectories of limb movements. As the output variables utility of non-linear methods, including neural networks [14– are continuous in these studies, a regression model is commonly 17], multilinear perceptrons [18], and support vector used. However, the decoding of limb movements is not a pure machines [18], but they tend to have difficulty with high regression problem, because the trajectories can be apparently dimensional features and limited training data [13]. classified into a motion state and a resting state, which result in a binary property overlooked by previous studies. In this Nevertheless, the studies of limb movement translation paper, we propose an algorithm called logistic-weighted are in fact not pure regression problems, because the limbs regression to make use of the property, and apply the algorithm are not always under the motion state. Whether it is during an to a BCI system decoding flexion of human fingers from ECoG experiment or in the daily life, the resting state of the limbs is signals. -
Lecture 19: Wavelet Compression of Time Series and Images
Lecture 19: Wavelet compression of time series and images c Christopher S. Bretherton Winter 2014 Ref: Matlab Wavelet Toolbox help. 19.1 Wavelet compression of a time series The last section of wavelet leleccum notoolbox.m demonstrates the use of wavelet compression on a time series. The idea is to keep the wavelet coefficients of largest amplitude and zero out the small ones. 19.2 Wavelet analysis/compression of an image Wavelet analysis is easily extended to two-dimensional images or datasets (data matrices), by first doing a wavelet transform of each column of the matrix, then transforming each row of the result (see wavelet image). The wavelet coeffi- cient matrix has the highest level (largest-scale) averages in the first rows/columns, then successively smaller detail scales further down the rows/columns. The ex- ample also shows fine results with 50-fold data compression. 19.3 Continuous Wavelet Transform (CWT) Given a continuous signal u(t) and an analyzing wavelet (x), the CWT has the form Z 1 s − t W (λ, t) = λ−1=2 ( )u(s)ds (19.3.1) −∞ λ Here λ, the scale, is a continuous variable. We insist that have mean zero and that its square integrates to 1. The continuous Haar wavelet is defined: 8 < 1 0 < t < 1=2 (t) = −1 1=2 < t < 1 (19.3.2) : 0 otherwise W (λ, t) is proportional to the difference of running means of u over successive intervals of length λ/2. 1 Amath 482/582 Lecture 19 Bretherton - Winter 2014 2 In practice, for a discrete time series, the integral is evaluated as a Riemann sum using the Matlab wavelet toolbox function cwt. -
Adaptive Wavelet Clustering for Highly Noisy Data
Adaptive Wavelet Clustering for Highly Noisy Data Zengjian Chen Jiayi Liu Yihe Deng Department of Computer Science Department of Computer Science Department of Mathematics Huazhong University of University of Massachusetts Amherst University of California, Los Angeles Science and Technology Massachusetts, USA California, USA Wuhan, China [email protected] [email protected] [email protected] Kun He* John E. Hopcroft Department of Computer Science Department of Computer Science Huazhong University of Science and Technology Cornell University Wuhan, China Ithaca, NY, USA [email protected] [email protected] Abstract—In this paper we make progress on the unsupervised Based on the pioneering work of Sheikholeslami that applies task of mining arbitrarily shaped clusters in highly noisy datasets, wavelet transform, originally used for signal processing, on which is a task present in many real-world applications. Based spatial data clustering [12], we propose a new wavelet based on the fundamental work that first applies a wavelet transform to data clustering, we propose an adaptive clustering algorithm, algorithm called AdaWave that can adaptively and effectively denoted as AdaWave, which exhibits favorable characteristics for uncover clusters in highly noisy data. To tackle general appli- clustering. By a self-adaptive thresholding technique, AdaWave cations, we assume that the clusters in a dataset do not follow is parameter free and can handle data in various situations. any specific distribution and can be arbitrarily shaped. It is deterministic, fast in linear time, order-insensitive, shape- To show the hardness of the clustering task, we first design insensitive, robust to highly noisy data, and requires no pre- knowledge on data models. -
A Fourier-Wavelet Monte Carlo Method for Fractal Random Fields
JOURNAL OF COMPUTATIONAL PHYSICS 132, 384±408 (1997) ARTICLE NO. CP965647 A Fourier±Wavelet Monte Carlo Method for Fractal Random Fields Frank W. Elliott Jr., David J. Horntrop, and Andrew J. Majda Courant Institute of Mathematical Sciences, 251 Mercer Street, New York, New York 10012 Received August 2, 1996; revised December 23, 1996 2 2H k[v(x) 2 v(y)] l 5 CHux 2 yu , (1.1) A new hierarchical method for the Monte Carlo simulation of random ®elds called the Fourier±wavelet method is developed and where 0 , H , 1 is the Hurst exponent and k?l denotes applied to isotropic Gaussian random ®elds with power law spectral the expected value. density functions. This technique is based upon the orthogonal Here we develop a new Monte Carlo method based upon decomposition of the Fourier stochastic integral representation of the ®eld using wavelets. The Meyer wavelet is used here because a wavelet expansion of the Fourier space representation of its rapid decay properties allow for a very compact representation the fractal random ®elds in (1.1). This method is capable of the ®eld. The Fourier±wavelet method is shown to be straightfor- of generating a velocity ®eld with the Kolmogoroff spec- ward to implement, given the nature of the necessary precomputa- trum (H 5 Ad in (1.1)) over many (10 to 15) decades of tions and the run-time calculations, and yields comparable results scaling behavior comparable to the physical space multi- with scaling behavior over as many decades as the physical space multiwavelet methods developed recently by two of the authors. -
Random Signals
Chapter 8 RANDOM SIGNALS Signals can be divided into two main categories - deterministic and random. The term random signal is used primarily to denote signals, which have a random in its nature source. As an example we can mention the thermal noise, which is created by the random movement of electrons in an electric conductor. Apart from this, the term random signal is used also for signals falling into other categories, such as periodic signals, which have one or several parameters that have appropriate random behavior. An example is a periodic sinusoidal signal with a random phase or amplitude. Signals can be treated either as deterministic or random, depending on the application. Speech, for example, can be considered as a deterministic signal, if one specific speech waveform is considered. It can also be viewed as a random process if one considers the ensemble of all possible speech waveforms in order to design a system that will optimally process speech signals, in general. The behavior of stochastic signals can be described only in the mean. The description of such signals is as a rule based on terms and concepts borrowed from probability theory. Signals are, however, a function of time and such description becomes quickly difficult to manage and impractical. Only a fraction of the signals, known as ergodic, can be handled in a relatively simple way. Among those signals that are excluded are the class of the non-stationary signals, which otherwise play an essential part in practice. Working in frequency domain is a powerful technique in signal processing. While the spectrum is directly related to the deterministic signals, the spectrum of a ran- dom signal is defined through its correlation function. -
A Practical Guide to Wavelet Analysis
A Practical Guide to Wavelet Analysis Christopher Torrence and Gilbert P. Compo Program in Atmospheric and Oceanic Sciences, University of Colorado, Boulder, Colorado ABSTRACT A practical step-by-step guide to wavelet analysis is given, with examples taken from time series of the El Niño– Southern Oscillation (ENSO). The guide includes a comparison to the windowed Fourier transform, the choice of an appropriate wavelet basis function, edge effects due to finite-length time series, and the relationship between wavelet scale and Fourier frequency. New statistical significance tests for wavelet power spectra are developed by deriving theo- retical wavelet spectra for white and red noise processes and using these to establish significance levels and confidence intervals. It is shown that smoothing in time or scale can be used to increase the confidence of the wavelet spectrum. Empirical formulas are given for the effect of smoothing on significance levels and confidence intervals. Extensions to wavelet analysis such as filtering, the power Hovmöller, cross-wavelet spectra, and coherence are described. The statistical significance tests are used to give a quantitative measure of changes in ENSO variance on interdecadal timescales. Using new datasets that extend back to 1871, the Niño3 sea surface temperature and the Southern Oscilla- tion index show significantly higher power during 1880–1920 and 1960–90, and lower power during 1920–60, as well as a possible 15-yr modulation of variance. The power Hovmöller of sea level pressure shows significant variations in 2–8-yr wavelet power in both longitude and time. 1. Introduction complete description of geophysical applications can be found in Foufoula-Georgiou and Kumar (1995), Wavelet analysis is becoming a common tool for while a theoretical treatment of wavelet analysis is analyzing localized variations of power within a time given in Daubechies (1992). -
An Overview of Wavelet Transform Concepts and Applications
An overview of wavelet transform concepts and applications Christopher Liner, University of Houston February 26, 2010 Abstract The continuous wavelet transform utilizing a complex Morlet analyzing wavelet has a close connection to the Fourier transform and is a powerful analysis tool for decomposing broadband wavefield data. A wide range of seismic wavelet applications have been reported over the last three decades, and the free Seismic Unix processing system now contains a code (succwt) based on the work reported here. Introduction The continuous wavelet transform (CWT) is one method of investigating the time-frequency details of data whose spectral content varies with time (non-stationary time series). Moti- vation for the CWT can be found in Goupillaud et al. [12], along with a discussion of its relationship to the Fourier and Gabor transforms. As a brief overview, we note that French geophysicist J. Morlet worked with non- stationary time series in the late 1970's to find an alternative to the short-time Fourier transform (STFT). The STFT was known to have poor localization in both time and fre- quency, although it was a first step beyond the standard Fourier transform in the analysis of such data. Morlet's original wavelet transform idea was developed in collaboration with the- oretical physicist A. Grossmann, whose contributions included an exact inversion formula. A series of fundamental papers flowed from this collaboration [16, 12, 13], and connections were soon recognized between Morlet's wavelet transform and earlier methods, including harmonic analysis, scale-space representations, and conjugated quadrature filters. For fur- ther details, the interested reader is referred to Daubechies' [7] account of the early history of the wavelet transform. -
STATISTICAL FOURIER ANALYSIS: CLARIFICATIONS and INTERPRETATIONS by DSG Pollock
STATISTICAL FOURIER ANALYSIS: CLARIFICATIONS AND INTERPRETATIONS by D.S.G. Pollock (University of Leicester) Email: stephen [email protected] This paper expounds some of the results of Fourier theory that are es- sential to the statistical analysis of time series. It employs the algebra of circulant matrices to expose the structure of the discrete Fourier transform and to elucidate the filtering operations that may be applied to finite data sequences. An ideal filter with a gain of unity throughout the pass band and a gain of zero throughout the stop band is commonly regarded as incapable of being realised in finite samples. It is shown here that, to the contrary, such a filter can be realised both in the time domain and in the frequency domain. The algebra of circulant matrices is also helpful in revealing the nature of statistical processes that are band limited in the frequency domain. In order to apply the conventional techniques of autoregressive moving-average modelling, the data generated by such processes must be subjected to anti- aliasing filtering and sub sampling. These techniques are also described. It is argued that band-limited processes are more prevalent in statis- tical and econometric time series than is commonly recognised. 1 D.S.G. POLLOCK: Statistical Fourier Analysis 1. Introduction Statistical Fourier analysis is an important part of modern time-series analysis, yet it frequently poses an impediment that prevents a full understanding of temporal stochastic processes and of the manipulations to which their data are amenable. This paper provides a survey of the theory that is not overburdened by inessential complications, and it addresses some enduring misapprehensions. -
Use of the Kurtosis Statistic in the Frequency Domain As an Aid In
lEEE JOURNALlEEE OF OCEANICENGINEERING, VOL. OE-9, NO. 2, APRIL 1984 85 Use of the Kurtosis Statistic in the FrequencyDomain as an Aid in Detecting Random Signals Absmact-Power spectral density estimation is often employed as a couldbe utilized in signal processing. The objective ofthis method for signal ,detection. For signals which occur randomly, a paper is to compare the PSD technique for signal processing frequency domain kurtosis estimate supplements the power spectral witha new methodwhich computes the frequency domain density estimate and, in some cases, can be.employed to detect their presence. This has been verified from experiments vith real data of kurtosis (FDK) [2] forthe real and imaginary parts of the randomly occurring signals. In order to better understand the detec- complex frequency components. Kurtosis is defined as a ratio tion of randomlyoccurring signals, sinusoidal and narrow-band of a fourth-order central moment to the square of a second- Gaussian signals are considered, which when modeled to represent a order central moment. fading or multipath environment, are received as nowGaussian in Using theNeyman-Pearson theory in thetime domain, terms of a frequency domain kurtosis estimate. Several fading and multipath propagation probability density distributions of practical Ferguson [3] , has shown that kurtosis is a locally optimum interestare considered, including Rayleigh and log-normal. The detectionstatistic under certain conditions. The reader is model is generalized to handle transient and frequency modulated referred to Ferguson'swork for the details; however, it can signals by taking into account the probability of the signal being in a be simply said thatit is concernedwith detecting outliers specific frequency range over the total data interval. -
2D Fourier, Scale, and Cross-Correlation
2D Fourier, Scale, and Cross-correlation CS 510 Lecture #12 February 26th, 2014 Where are we? • We can detect objects, but they can only differ in translation and 2D rotation • Then we introduced Fourier analysis. • Why? – Because Fourier analysis can help us with scale – Because Fourier analysis can make correlation faster Review: Discrete Fourier Transform • Problem: an image is not an analogue signal that we can integrate. • Therefore for 0 ≤ x < N and 0 ≤ u <N/2: N −1 * # 2πux & # 2πux &- F(u) = ∑ f (x),cos % ( − isin% (/ x=0 + $ N ' $ N '. And the discrete inverse transform is: € 1 N −1 ) # 2πux & # 2πux &, f (x) = ∑F(u)+cos % ( + isin% (. N x=0 * $ N ' $ N '- CS 510, Image Computaon, ©Ross 3/2/14 3 Beveridge & Bruce Draper € 2D Fourier Transform • So far, we have looked only at 1D signals • For 2D signals, the continuous generalization is: ∞ ∞ F(u,v) ≡ ∫ ∫ f (x, y)[cos(2π(ux + vy)) − isin(2π(ux + vy))] −∞ −∞ • Note that frequencies are now two- dimensional € – u= freq in x, v = freq in y • Every frequency (u,v) has a real and an imaginary component. CS 510, Image Computaon, ©Ross 3/2/14 4 Beveridge & Bruce Draper 2D sine waves • This looks like you’d expect in 2D Ø Note that the frequencies don’t have to be equal in the two dimensions. hp://images.google.com/imgres?imgurl=hFp://developer.nvidia.com/dev_content/cg/cg_examples/images/ sine_wave_perturbaon_ogl.jpg&imgrefurl=hFp://developer.nvidia.com/object/ cg_effects_explained.html&usg=__0FimoxuhWMm59cbwhch0TLwGpQM=&h=350&w=350&sz=13&hl=en&start=8&sig2=dBEtH0hp5I1BExgkXAe_kg&tbnid=fc yrIaap0P3M:&tbnh=120&tbnw=120&ei=llCYSbLNL4miMoOwoP8L&prev=/images%3Fq%3D2D%2Bsine%2Bwave%26gbv%3D2%26hl%3Den%26sa%3DG CS 510, Image Computaon, ©Ross 3/2/14 5 Beveridge & Bruce Draper 2D Discrete Fourier Transform N /2 N /2 * # 2π & # 2π &- F(u,v) = ∑ ∑ f (x, y),cos % (ux + vy)( − isin% (ux + vy)(/ x=−N /2 y=−N /2 + $ N ' $ N '.