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Lesson 9 Introduction Signal Spectral Analysis: Estimation of the power spectral density The problem of spectral estimation is very large and has applications very different from each other Applications: To study the vibrations of


  1. Lesson 9

  2. Introduction  Signal Spectral Analysis: Estimation of the power spectral density  The problem of spectral estimation is very large and has applications very different from each other  Applications:  To study the vibrations of a system  To study the stability of the frequency of a oscillator  To estimate the position and number of signal sources in an acoustic field  To estimate the parameters of the vocal tract of a speaker  Medical diagnosis  Control system design  In general To estimate and predict signals in time or in space

  3. Study of radio frequency spectrum in a big city  side by side there are the various radio and television channels, the signals cell phone, radar signals, etc.  The frequency ranges, if considered with sufficient bandwidth, are occupied by signals totally independent of each other, with different amplitudes and different statistical characteristics  To analyze the spectrum, it seems logical to use a selective receiver that measures the energy content in each interval frequency. Non Parametric  We will seek the most accurate possible Spectral Analysis estimate of these energies in the time available without making any further assumptions, not looking for models of signal generation

  4. Study of radio frequency spectrum in a big city  The non-parametric spectral analysis is a conceptually simple matter if you use the concept of ensemble average.  if you have enough realizations of the signal, just calculate the discrete Fourier transform and averaging the powers, component by component.  However, rarely you have numerous replicas of the signal; often, you have available a single replica, for an interval of time allotted  To determine the power spectrum, you have to use additional assumptions such as stationarity and ergodicity

  5. Analysis of the speech signal  consider the spectrum of acoustic signal due to vibration or a voice signal  in this case, all of the signal as a whole has unique origins and then there will be the relationship between the contents of the various spectral bands.  it must first choose a model for the generation of the signal and then determine Parametric the parameters of the model itself Spectral Analysis  For example, it will seek the parameters of a linear filter that, powered by a uniform spectrum signal (white noise) produces a power spectrum similar to the spectrum under analysis

  6. Analysis of the speech signal  Obviously, the success of the technique depends on the quality and parametric correctness of the model chosen.  Valid models lead to a parsimonious signal description , that is characterized by the minimum number of parameters necessary  This will lead to a better estimate of these parameters and then to optimal results  the parametric spectral analysis leads to the identification of the model and this opens a subsequent phase of study to understand and then possibly check the status and evolution the system under observation

  7. Formal Problem Definition  Let be y= {y(1), y(2), . . . , y(N)} a second order stationary random process, ˆ    GOAL: to determine an estimate of its power ( ) spectral density for ω ∈ [−π, +π ]  (  )  Observation ˆ        We want | ( ) ( ) | 0  The main limitation on the quality of most PSD estimates is due to the quite small number of data samples N usually available  Most commonly, N is limited by the fact that the signal under study can be considered wide sense stationary only over short observation intervals

  8. Two possible way(1)  There are two main approaches Non Parametric Parametric Spectral Spectral Analysis Analysis assume that the underlying stationary explicitly estimate the covariance stochastic process has a certain structure or the spectrum of the process which can be described using a small without assuming that the number of parameters. In these approaches, process has any particular the task is to estimate the parameters of the structure model that describes the stochastic process

  9. Non Parametric Estimation: Priodogram  The periodogram method was introduced by Schuster in 1898.  The periodogram method relies on the definition of the PSD  in practice the signal y(t) is only available for a finite interval Periodogram Power Specrtal Density Estimation

  10. Correlogram  Spectrum estimation can be interpreted as an autocorrelation estimation problem. Correlogram Power Specrtal Density Estimation the estimate of the covariance lag r(k), obtained from the available sample {y(1), y(2), . . . , y(N)}

  11. Estimation of Autocorrelation Sequence(ACS)  There are two standard way to obtain an estimate ˆ k ( ) r  unbiased estimate  biased estimate  Both estimators respect the symmetry properties of the ACS  The biased estimate is usually preferred, for the following reasons:  the ACS sequence decays rather rapidly so that r(k) is quite small for large lags k  the ACS sequence is guaranteed to be positive semidefinite . is not the case for the unbised definition  if the biased ACS estimator is used in the estimation the correlogram is eqaul to the periodogramm

  12. Statistical Performance  Both Periodogram and Correlogram are asymptotically unbiased:  Both have large variance, even for large N  ˆ  can be large for big k | ( ) ( ) | r k r k  ˆ | ( ) ( ) | r k r k  even if the errors are small, there are ”so many” ˆ    that when summed in the PSD error is large | ( ) ( ) | k k

  13. Periodogram Bias Bartlett window. Frequency Domain

  14. Bartlett window  Ideally, to have zero bias, we want WB(ω ) = Dirac impulse δ(ω )  The main lobe width decreases as 1/N.  For small values of N, WB(ω) may differ quite a bit from δ(ω )  If the unbised estimation the window is rectangular

  15. Summary Bias analysis  Note that, unlike WB(ω ), WR(ω ) can assume negative values for some values of ω, thus providing estimate of the PSD that can be negative for some frequencies.  The bias manifests itself in different ways  Main lobe width causes smearing (or smooting): details in φ(ω) separated in f by less than 1/N are not resolvable.  periodogram resolution limit = 1/N  Sidelobe level causes leakage  For small N, severe bias  As N → ∞, WB (ω) → δ(ω), so φ(ω ) is asymptotically unbiased

  16. Periodogram Variance  As N → ∞  inconsistent estimate  erratic behavior

  17. The Blackman-Tukey method  Basic idea : weighted correlogram , with small weight applied to the estimated covariances r(k) with large k lag window Frequency Domain  The BT periodogram is a locally smoothed  Variance decreases substantially (of the order of M/N)  Bias increases slightly (of the order 1/M)  The window is chosen so as to ensure that the spectral density of estimated power is always positive

  18. Choice of the BT window  Let be  It is possible to prove that  This means that the more slowly the window decays to zero in one domain, the more concentrated it is in the other domain  The equivalent temporal width, N e is determined by the window length (Ne = 2M) for rectangular window, Ne = M for triangular window).  Since N e βe = 1 also the bandwidth β e is determined by the window length  As M increases, bias decreases and variance increases ⇒ choose M as a tradeoff between variance and bias. As a rule of thumb, we should choose M ≤ N/ 10 in order to reduce the standard deviation of the estimated spectrum at least three times, compared with the periodogram  Choose window shape to compromise between smearing (main lobe width) and leakage (sidelobe level). The energy in the main lobe and in the sidelobes cannot be reduced simultaneously, once M is given

  19. The Bartlett method  Basic idea : split up the available sample of N observations into L = N/M subsamples of M observations each, then average the periodograms obtained from the subsamples for each value of ω.

  20. Welch method  Similar to Bartlett method, but allow overlap of subsequences (gives more subsequences, thus better averaging) and use data window for each periodogram; gives mainlobe-sidelobe tradeoff capability overlap  if K = M, no overlap as in Bartlett method  if K = M/2, 50% overlap, S = 2M/N data segments  The Welch method is approximately equal to Blackman- Tuckey with a non-rectangular lag window

  21. Daniell  It can be proved that, for are nearly uncorrelated random variables for  The basic idea of the Daniel method is to perform local averaging of 2J + 1 samples in the frequency domain to reduce the variance by about 2J + 1  As J increases:  bias increases (more smoothing)  variance decreases (more averaging)

  22. Non parametric estimation summary  The non-parametric spectral analysis is a conceptually simple matter if you use the concept of ensemble average  Goal is to estimate the covariance or the spectrum of the process without assuming that the process has any particular structure  Priodogram- Correlogram  Asymptotically unbiased, inconsistence  None of the methods we have seen solves all the problems of the periodogram  Parametic estimation…

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