Windowing Design and Performance Assessment for Mitigation of Spectrum Leakage
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Spectrum Estimation Using Periodogram, Bartlett and Welch
Spectrum estimation using Periodogram, Bartlett and Welch Guido Schuster Slides follow closely chapter 8 in the book „Statistical Digital Signal Processing and Modeling“ by Monson H. Hayes and most of the figures and formulas are taken from there 1 Introduction • We want to estimate the power spectral density of a wide- sense stationary random process • Recall that the power spectrum is the Fourier transform of the autocorrelation sequence • For an ergodic process the following holds 2 Introduction • The main problem of power spectrum estimation is – The data x(n) is always finite! • Two basic approaches – Nonparametric (Periodogram, Bartlett and Welch) • These are the most common ones and will be presented in the next pages – Parametric approaches • not discussed here since they are less common 3 Nonparametric methods • These are the most commonly used ones • x(n) is only measured between n=0,..,N-1 • Ensures that the values of x(n) that fall outside the interval [0,N-1] are excluded, where for negative values of k we use conjugate symmetry 4 Periodogram • Taking the Fourier transform of this autocorrelation estimate results in an estimate of the power spectrum, known as the Periodogram • This can also be directly expressed in terms of the data x(n) using the rectangular windowed function xN(n) 5 Periodogram of white noise 32 samples 6 Performance of the Periodogram • If N goes to infinity, does the Periodogram converge towards the power spectrum in the mean squared sense? • Necessary conditions – asymptotically unbiased: – variance -
Configuring Spectrogram Views
Chapter 5: Spectrographic Analysis Configuring spectrographic views To create a new spectrogram, spectrogram slice, or selection spectrum view, click on the appropriate New View button in the view toolbar (Figure 5.3) or choose a view type from the View > New menu. Figure 5.3. New View buttons Figure 5.3. The New View buttons, in Raven’s view toolbar. 112 Raven Pro 1.4 User’s Manual Chapter 5: Spectrographic Analysis A dialog box appears, containing parameters for configuring the requested type of spectrographic view (Figure 5.4). The dialog boxes for configuring spectrogram and spectrogram slice views are identical, except for their titles. The dialog boxes are identical because both view types calculate a spectrogram of the entire sound; the only difference between spectrogram and spectrogram slice views is in how the data are displayed (see “How the spectrographic views are related” on page 110). The dialog box for configuring a selection spectrum view is the same, except that it lacks the Averaging parameter. The remainder of this section explains each of the parameters in the configuration dialog box. Figure 5.4 Configure Spectrogram dialog Figure 5.4. The Configure New Spectrogram dialog box. Window type Each data record is multiplied by a window function before its spectrum is calculated. Window functions are used to reduce the magnitude of spurious “sidelobe” energy that appears at frequencies flanking each analysis frequency in a spectrum. These sidelobes appear as a result of Raven Pro 1.4 User’s Manual 113 Chapter 5: Spectrographic Analysis analyzing a finite (truncated) portion of a signal. -
An Information Theoretic Algorithm for Finding Periodicities in Stellar Light Curves Pablo Huijse, Student Member, IEEE, Pablo A
IEEE TRANSACTIONS ON SIGNAL PROCESSING, VOL. 1, NO. 1, JANUARY 2012 1 An Information Theoretic Algorithm for Finding Periodicities in Stellar Light Curves Pablo Huijse, Student Member, IEEE, Pablo A. Estevez*,´ Senior Member, IEEE, Pavlos Protopapas, Pablo Zegers, Senior Member, IEEE, and Jose´ C. Pr´ıncipe, Fellow Member, IEEE Abstract—We propose a new information theoretic metric aligned to Earth. Periodic drops in brightness are observed for finding periodicities in stellar light curves. Light curves due to the mutual eclipses between the components of the are astronomical time series of brightness over time, and are system. Although most stars have at least some variation in characterized as being noisy and unevenly sampled. The proposed metric combines correntropy (generalized correlation) with a luminosity, current ground based survey estimations indicate periodic kernel to measure similarity among samples separated that 3% of the stars varying more than the sensitivity of the by a given period. The new metric provides a periodogram, called instruments and ∼1% are periodic [2]. Correntropy Kernelized Periodogram (CKP), whose peaks are associated with the fundamental frequencies present in the data. Detecting periodicity and estimating the period of stars is The CKP does not require any resampling, slotting or folding of high importance in astronomy. The period is a key feature scheme as it is computed directly from the available samples. for classifying variable stars [3], [4]; and estimating other CKP is the main part of a fully-automated pipeline for periodic light curve discrimination to be used in astronomical survey parameters such as mass and distance to Earth [5]. -
Windowing Techniques, the Welch Method for Improvement of Power Spectrum Estimation
Computers, Materials & Continua Tech Science Press DOI:10.32604/cmc.2021.014752 Article Windowing Techniques, the Welch Method for Improvement of Power Spectrum Estimation Dah-Jing Jwo1, *, Wei-Yeh Chang1 and I-Hua Wu2 1Department of Communications, Navigation and Control Engineering, National Taiwan Ocean University, Keelung, 202-24, Taiwan 2Innovative Navigation Technology Ltd., Kaohsiung, 801, Taiwan *Corresponding Author: Dah-Jing Jwo. Email: [email protected] Received: 01 October 2020; Accepted: 08 November 2020 Abstract: This paper revisits the characteristics of windowing techniques with various window functions involved, and successively investigates spectral leak- age mitigation utilizing the Welch method. The discrete Fourier transform (DFT) is ubiquitous in digital signal processing (DSP) for the spectrum anal- ysis and can be efciently realized by the fast Fourier transform (FFT). The sampling signal will result in distortion and thus may cause unpredictable spectral leakage in discrete spectrum when the DFT is employed. Windowing is implemented by multiplying the input signal with a window function and windowing amplitude modulates the input signal so that the spectral leakage is evened out. Therefore, windowing processing reduces the amplitude of the samples at the beginning and end of the window. In addition to selecting appropriate window functions, a pretreatment method, such as the Welch method, is effective to mitigate the spectral leakage. Due to the noise caused by imperfect, nite data, the noise reduction from Welch’s method is a desired treatment. The nonparametric Welch method is an improvement on the peri- odogram spectrum estimation method where the signal-to-noise ratio (SNR) is high and mitigates noise in the estimated power spectra in exchange for frequency resolution reduction. -
Discrete-Time Fourier Transform
.@.$$-@@4&@$QEG'FC1. CHAPTER7 Discrete-Time Fourier Transform In Chapter 3 and Appendix C, we showed that interesting continuous-time waveforms x(t) can be synthesized by summing sinusoids, or complex exponential signals, having different frequencies fk and complex amplitudes ak. We also introduced the concept of the spectrum of a signal as the collection of information about the frequencies and corresponding complex amplitudes {fk,ak} of the complex exponential signals, and found it convenient to display the spectrum as a plot of spectrum lines versus frequency, each labeled with amplitude and phase. This spectrum plot is a frequency-domain representation that tells us at a glance “how much of each frequency is present in the signal.” In Chapter 4, we extended the spectrum concept from continuous-time signals x(t) to discrete-time signals x[n] obtained by sampling x(t). In the discrete-time case, the line spectrum is plotted as a function of normalized frequency ωˆ . In Chapter 6, we developed the frequency response H(ejωˆ ) which is the frequency-domain representation of an FIR filter. Since an FIR filter can also be characterized in the time domain by its impulse response signal h[n], it is not hard to imagine that the frequency response is the frequency-domain representation,orspectrum, of the sequence h[n]. 236 .@.$$-@@4&@$QEG'FC1. 7-1 DTFT: FOURIER TRANSFORM FOR DISCRETE-TIME SIGNALS 237 In this chapter, we take the next step by developing the discrete-time Fouriertransform (DTFT). The DTFT is a frequency-domain representation for a wide range of both finite- and infinite-length discrete-time signals x[n]. -
Understanding the Lomb-Scargle Periodogram
Understanding the Lomb-Scargle Periodogram Jacob T. VanderPlas1 ABSTRACT The Lomb-Scargle periodogram is a well-known algorithm for detecting and char- acterizing periodic signals in unevenly-sampled data. This paper presents a conceptual introduction to the Lomb-Scargle periodogram and important practical considerations for its use. Rather than a rigorous mathematical treatment, the goal of this paper is to build intuition about what assumptions are implicit in the use of the Lomb-Scargle periodogram and related estimators of periodicity, so as to motivate important practical considerations required in its proper application and interpretation. Subject headings: methods: data analysis | methods: statistical 1. Introduction The Lomb-Scargle periodogram (Lomb 1976; Scargle 1982) is a well-known algorithm for de- tecting and characterizing periodicity in unevenly-sampled time-series, and has seen particularly wide use within the astronomy community. As an example of a typical application of this method, consider the data shown in Figure 1: this is an irregularly-sampled timeseries showing a single ob- ject from the LINEAR survey (Sesar et al. 2011; Palaversa et al. 2013), with un-filtered magnitude measured 280 times over the course of five and a half years. By eye, it is clear that the brightness of the object varies in time with a range spanning approximately 0.8 magnitudes, but what is not immediately clear is that this variation is periodic in time. The Lomb-Scargle periodogram is a method that allows efficient computation of a Fourier-like power spectrum estimator from such unevenly-sampled data, resulting in an intuitive means of determining the period of oscillation. -
Effect of Data Gaps: Comparison of Different Spectral Analysis Methods
Ann. Geophys., 34, 437–449, 2016 www.ann-geophys.net/34/437/2016/ doi:10.5194/angeo-34-437-2016 © Author(s) 2016. CC Attribution 3.0 License. Effect of data gaps: comparison of different spectral analysis methods Costel Munteanu1,2,3, Catalin Negrea1,4,5, Marius Echim1,6, and Kalevi Mursula2 1Institute of Space Science, Magurele, Romania 2Astronomy and Space Physics Research Unit, University of Oulu, Oulu, Finland 3Department of Physics, University of Bucharest, Magurele, Romania 4Cooperative Institute for Research in Environmental Sciences, Univ. of Colorado, Boulder, Colorado, USA 5Space Weather Prediction Center, NOAA, Boulder, Colorado, USA 6Belgian Institute of Space Aeronomy, Brussels, Belgium Correspondence to: Costel Munteanu ([email protected]) Received: 31 August 2015 – Revised: 14 March 2016 – Accepted: 28 March 2016 – Published: 19 April 2016 Abstract. In this paper we investigate quantitatively the ef- 1 Introduction fect of data gaps for four methods of estimating the ampli- tude spectrum of a time series: fast Fourier transform (FFT), Spectral analysis is a widely used tool in data analysis and discrete Fourier transform (DFT), Z transform (ZTR) and processing in most fields of science. The technique became the Lomb–Scargle algorithm (LST). We devise two tests: the very popular with the introduction of the fast Fourier trans- single-large-gap test, which can probe the effect of a sin- form algorithm which allowed for an extremely rapid com- gle data gap of varying size and the multiple-small-gaps test, putation of the Fourier Transform. In the absence of modern used to study the effect of numerous small gaps of variable supercomputers, this was not just useful, but also the only size distributed within the time series. -
Optimal and Adaptive Subband Beamforming
Optimal and Adaptive Subband Beamforming Principles and Applications Nedelko Grbi´c Ronneby, June 2001 Department of Telecommunications and Signal Processing Blekinge Institute of Technology, S-372 25 Ronneby, Sweden c Nedelko Grbi´c ISBN 91-7295-002-1 ISSN 1650-2159 Published 2001 Printed by Kaserntryckeriet AB Karlskrona 2001 Sweden v Preface This doctoral thesis summarizes my work in the field of array signal processing. Frequency domain processing comprise a significant part of the material. The work is mainly aimed at speech enhancement in communication systems such as confer- ence telephony and handsfree mobile telephony. The work has been carried out at Department of Telecommunications and Signal Processing at Blekinge Institute of Technology. Some of the work has been conducted in collaboration with Ericsson Mobile Communications and Australian Telecommunications Research Institute. The thesis consists of seven stand alone parts: Part I Optimal and Adaptive Beamforming for Speech Signals Part II Structures and Performance Limits in Subband Beamforming Part III Blind Signal Separation using Overcomplete Subband Representation Part IV Neural Network based Adaptive Microphone Array System for Speech Enhancement Part V Design of Oversampled Uniform DFT Filter Banks with Delay Specifica- tion using Quadratic Optimization Part VI Design of Oversampled Uniform DFT Filter Banks with Reduced Inband Aliasing and Delay Constraints Part VII A New Pilot-Signal based Space-Time Adaptive Algorithm vii Acknowledgments I owe sincere gratitude to Professor Sven Nordholm with whom most of my work has been conducted. There have been enormous amount of inspiration and valuable discussions with him. Many thanks also goes to Professor Ingvar Claesson who has made every possible effort to make my study complete and rewarding. -
Airborne Radar Ground Clutter Suppression Using Multitaper Spectrum Estimation Comparison with Traditional Method
Airborne Radar Ground Clutter Suppression Using Multitaper Spectrum Estimation Comparison with Traditional Method Linus Ekvall Engineering Physics and Electrical Engineering, master's level 2018 Luleå University of Technology Department of Computer Science, Electrical and Space Engineering Airborne Radar Ground Clutter Suppression Using Multitaper Spectrum Estimation & Comparison with Traditional Method Linus C. Ekvall Lule˚aUniversity of Technology Dept. of Computer Science, Electrical and Space Engineering Div. Signals and Systems 20th September 2018 ABSTRACT During processing of data received by an airborne radar one of the issues is that the typical signal echo from the ground produces a large perturbation. Due to this perturbation it can be difficult to detect targets with low velocity or a low signal-to-noise ratio. Therefore, a filtering process is needed to separate the large perturbation from the target signal. The traditional method include a tapered Fourier transform that operates in parallel with a MTI filter to suppress the main spectral peak in order to produce a smoother spectral output. The difference between a typical signal echo produced from an object in the environment and the signal echo from the ground can be of a magnitude corresponding to more than a 60 dB difference. This thesis presents research of how the multitaper approach can be utilized in concurrence with the minimum variance estimation technique, to produce a spectral estimation that strives for a more effective clutter suppression. A simulation model of the ground clutter was constructed and also a number of simulations for the multitaper, minimum variance estimation technique was made. Compared to the traditional method defined in this thesis, there was a slight improve- ment of the improvement factor when using the multitaper approach. -
Chapter 2: the Fourier Transform Chapter 2
“EEE305”, “EEE801 Part A”: Digital Signal Processing Chapter 2: The Fourier Transform Chapter 2 The Fourier Transform 2.1 Introduction The sampled Fourier transform of a periodic, discrete-time signal is known as the discrete Fourier transform (DFT). The DFT of such a signal allows an interpretation of the frequency domain descriptions of the given signal. 2.2 Derivation of the DFT The Fourier transform pair of a continuous-time signal is given by Equation 2.1 and Equation 2.2. ∞ − j2πft X ( f ) = ∫ x(t) ⋅e dt (2.1) −∞ ∞ j2πft x(t) = ∫ X ( f ) ⋅e df (2.2) −∞ Now consider the signal x(t) to be periodic i.e. repeating. The Fourier transform pair from above can now be represented by Equation 2.3 and Equation 2.4 respectively. T0 1 − π = ⋅ j2 kf0t X (kf 0 ) ∫ x(t) e dt (2.3) T0 0 ∞ π = ⋅ j 2 kf0t x(t) ∑ X (kf0 ) e (2.4) k=−∞ = 1 where f 0 . Now suppose that the signal x(t) is sampled N times per period, as illustrated in Figure 2.1, with a T0 sampling period of T seconds. The discrete signal can now be represented by Equation 2.5, where δ is the dirac delta impulse function and has a unit area of one. ∞ x[nT ] = ∑ x(t) ⋅δ (t − nT ) (2.5) n=−∞ Now replace x(t) in the Fourier integral of Equation 2.3, with x[nT] of Equation 2.5. The Equation can now be re- written as: ∞ T0 1 − π = ⋅δ − ⋅ jk 2 f0t X (kf0 ) ∑ ∫ x(t) (t nT ) e dt (2.6) T0 n=−∞ 0 1 for t = nT Since the dirac delta function δ ()t − nT = , Equation 2.6 can be modified even further to become 0 otherwise Equation 2.7 below: N −1 1 − π = ⋅ jk 2 f0nT X[kf 0 ] ∑ x[nT] e (2.7) N n=0 University of Newcastle upon Tyne Page 2.1 “EEE305”, “EEE801 Part A”: Digital Signal Processing Chapter 2: The Fourier Transform Sampled sequence δ(t-nT) litude p Am nT Time (t) Figure 2.1: Sampled sequence for the DFT. -
The Sliding Window Discrete Fourier Transform Lee F
The Sliding Window Discrete Fourier Transform Lee F. Richardson Department of Statistics and Data Science, Carnegie Mellon University, Pittsburgh, PA The Sliding Window DFT Sliding Window DFT for Local Periodic Signals Leakage The Sliding Window Discrete Fourier Transform (SW- Leakage occurs when local signal frequency is not one DFT) computes a time-frequency representation of a The Sliding Window DFT is a useful tool for analyzing data with local periodic signals (Richardson and Eddy of the Fourier frequencies (or, the number of complete signal, and is useful for analyzing signals with local (2018)). Since SW-DFT coefficients are complex-numbers, we analyze the squared modulus of these coefficients cycles in a length n window is not an integer). In this periodicities. Shortly described, the SW-DFT takes 2 2 2 case, the largest squared modulus coefficients occur at sequential DFTs of a signal multiplied by a rectangu- |ak,p| = Re(ak,p) + Im(ak,p) frequencies closest to the true frequency: lar sliding window function, where the window func- Since the squared modulus SW-DFT coefficients are large when the window is on a periodic part of the signal: Frequency: 2 Frequency: 2.1 Frequency: 2.2 Frequency: 2.3 Frequency: 2.4 20 Freq 2 20 Freq 2 20 Freq 2 20 Freq 2 20 Freq 2 tion is only nonzero for a short duration. Let x = Freq 3 Freq 3 Freq 3 Freq 3 Freq 3 15 15 15 15 15 [x0, x1, . , xN−1] be a length N signal, then for length 10 10 10 10 10 n ≤ N windows, the SW-DFT of x is: 5 5 5 5 5 0 0 0 0 0 0 50 100 150 200 250 0 50 100 150 200 250 0 50 100 150 200 250 0 50 100 150 200 250 0 50 100 150 200 250 1 n−1 X −jk Frequency: 2.5 Frequency: 2.6 Frequency: 2.7 Frequency: 2.8 Frequency: 2.9 ak,p = √ xp−n+1+jω 20 Freq 2 20 Freq 2 20 Freq 2 20 Freq 2 20 Freq 2 n n Freq 3 Freq 3 Freq 3 Freq 3 Freq 3 j=0 15 15 15 15 15 k = 0, 1, . -
Topics in Time-Frequency Analysis
Kernels Multitaper basics MT spectrograms Concentration Topics in time-frequency analysis Maria Sandsten Lecture 7 Stationary and non-stationary spectral analysis February 10 2020 1 / 45 Kernels Multitaper basics MT spectrograms Concentration Wigner distribution The Wigner distribution is defined as, Z 1 τ ∗ τ −i2πf τ Wz (t; f ) = z(t + )z (t − )e dτ; −∞ 2 2 with t is time, f is frequency and z(t) is the analytic signal. The ambiguity function is defined as Z 1 τ ∗ τ −i2πνt Az (ν; τ) = z(t + )z (t − )e dt; −∞ 2 2 where ν is the doppler frequency and τ is the lag variable. 2 / 45 Kernels Multitaper basics MT spectrograms Concentration Ambiguity function Facts about the ambiguity function: I The auto-terms are always centered at ν = τ = 0. I The phase of the ambiguity function oscillations are related to centre t0 and f0 of the signal. I jAz1 (ν; τ)j = jAz0 (ν; τ)j when Wz1 (t; f ) = Wz0 (t − t0; f − f0). I The cross-terms are always located away from the centre. I The placement of the cross-terms are related to the interconnection of the auto-terms. 3 / 45 Kernels Multitaper basics MT spectrograms Concentration The quadratic class The quadratic or Cohen's class is usually defined as Z 1 Z 1 Z 1 Q τ ∗ τ i2π(νt−f τ−νu) Wz (t; f ) = z(u+ )z (u− )φ(ν; τ)e du dτ dν: −∞ −∞ −∞ 2 2 The filtered ambiguity function can also be formulated as Q Az (ν; τ) = Az (ν; τ) · φ(ν; τ); and the corresponding smoothed Wigner distribution as Q Wz (t; f ) = Wz (t; f ) ∗ ∗Φ(t; f ); using the corresponding time-frequency kernel.