Skip to content Skip to navigation

Connexions

You are here: Home » Content » Partially Known Signal Waveform

Navigation

Content Actions

  • Download module PDF
  • Add to ...
    Add the module to:
    • My Favorites
    • A lens
    • An external social bookmarking service
    • My Favorites (What is 'My Favorites'?)
      'My Favorites' is a special kind of lens which you can use to bookmark modules and collections directly in Connexions. 'My Favorites' can only be seen by you, and collections saved in 'My Favorites' can remember the last module you were on. You need a Connexions account to use 'My Favorites'.
    • A lens (What is a lens?)

      Definition of a lens

      Lenses

      A lens is a custom view of Connexions content. You can think of it as a fancy kind of list that will let you see Connexions through the eyes of organizations and people you trust.

      What is in a lens?

      Lens makers point to Connexions materials (modules and collections), creating a guide that includes their own comments and descriptive tags about the content.

      Who can create a lens?

      Any individual Connexions member, a community, or a respected organization.

    • External bookmarks
  • E-mail the author

Recently Viewed

Partially Known Signal Waveform

Module by: Don Johnson

The nominal signal waveform is known, but the actual signal present in the observed data can be corrupted slightly. Using the minimax approach, we seek the worst possible signal that could be present consistent with constraints on the corruption. Once we know what signal that is, our detector should consist of a filter matched to that worst-case signal. Let the observed signal be of the form sl= s o l+cl s l s o l c l : s o l s o l is the nominal signal and cl c l the corruption in the observed signal. The nominal-signal energy is E o E o and the signal corruption is assumed to have an energy that is less than E c E c . Spectral techniques are assumed to be applicable so that the covariance matrix of the Fourier transformed noise is diagonal. The signal-to-noise ratio is given by k|Sk|2 σ k 2 k S k 2 σ k 2 . What corruption yields the smallest signal-to-noise ratio? The worst-case signal will have the largest amount of corruption possible. This constrained minimization problem - minimize the signal-to-noise ratio while forcing the energy of the corruption to be less than E c E c - can then be solved using Lagrange multipliers. min S k {k|Sk|2 σ k 2+λk|Ck|2- E c } S k k S k 2 σ k 2 λ k C k 2 E c By evaluating the appropriate derivatives, we find the spectrum of the worst-case signal to be a frequency-weighted version of the nominal signal's spectrum. S w k=λ σ k 21+λ σ k 2 S o k S w k λ σ k 2 1 λ σ k 2 S o k where k11+λ σ k 22| S o k|2= E c k 1 1 λ σ k 2 2 S o k 2 E c The only unspecifies parameter is the Lagrange multiplier λλ, with the latter equation providing an implicit solution in most cases.

If the noise is white, the σ k 2 σ k 2 equal a constant, implying that the worst-case signal is a scaled version of the nominal, equaling S w k=1- E c E o S o k S w k 1 E c E o S o k . The robust decision rule derived from the likelihood ratio is given by k=0L-1Rk¯ S o k 0 1 γ k L 1 0 R k S o k 0 1 γ By incorporating the scaling constant 1- E c E o 1 E c E o into the threshold γγ, we find that the matched filter used in the white noise, known-signal case is robust with respect to signal uncertainties. The threshold value is identical to that derived using the nominal signal as model 0 0 does not depend on the uncertainties in the signal model. Thus, the detector used in the known-signal, white noise case can also be used when the signal is partially corrupted. Note that in solving the general signal corruption case, the imprecise signal amplitude situation was also solved.

If the noise is not white, the proportion between the nominal and worst-case signal spectral components is not a constant. The decision rule expressed in term of the frequency-domain sufficient statistic becomes k=0L-1λ σ k 21+λ σ k 2Rk¯ S o k 0 1 γ k L 1 0 λ σ k 2 1 λ σ k 2 R k S o k 0 1 γ Thus, the detector derived for colored noise problems is not robust. The threshold depends on the noise spectrum and the energy of the corruption. Furthermore, calculating the value of the Lagrange multiplier in the colored noise problem is quite difficult, with multiple solutions to its constraint equation quite possible. Only one of these solutions will correspond to the worst-case signal.

Comments, questions, feedback, criticisms?

Send feedback