2006
DOI: 10.1007/s00348-006-0199-5
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On spectral linear stochastic estimation

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Cited by 150 publications
(118 citation statements)
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“…On the other hand, the frequency spectrum of the axial velocity fluctuations near the nozzle lip for a turbulent jet is known to be flat up to St D ≈ 0.5. 33,34 This observation is used to scale the PSE solutions for m = 0 such that their axial velocity components are unity at (x = 0.5D, r = 0.5D). The resulting pressure amplitudes for the different frequencies at the location of the near-field linear array are shown in Figure 6(b).…”
Section: B Comparison With Pse Analysismentioning
confidence: 99%
“…On the other hand, the frequency spectrum of the axial velocity fluctuations near the nozzle lip for a turbulent jet is known to be flat up to St D ≈ 0.5. 33,34 This observation is used to scale the PSE solutions for m = 0 such that their axial velocity components are unity at (x = 0.5D, r = 0.5D). The resulting pressure amplitudes for the different frequencies at the location of the near-field linear array are shown in Figure 6(b).…”
Section: B Comparison With Pse Analysismentioning
confidence: 99%
“…Kernel H is equal to the inputoutput cross-spectrum, divided by the input spectrum, and may be expressed in terms of a gain, |H(z; f )|, and phase, φ(z; f ). Intuitively, the gain is the scaling factor for each Fourier mode during a linear stochastic estimate of the output [39][40][41], whereas the scale-dependent phase accounts …”
Section: (B) Conditional Structure and Inclinationmentioning
confidence: 99%
“…In contrast, [7], [17] proposed to take into account integrated temporal data by assuming a linear dependence between the modal coefficients and the flow measurements in a non-local way, by working in the frequency domain. Letα be the Fourier transform of α andf j that of f j , then for each frequency we poseα j = Ns k=1Γ kjfk (10) whereΓ kj is a matrix obtained by appropriate ensemble averages and depends on the frequency.…”
Section: Non-linear Observermentioning
confidence: 99%