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High-resolution Interferometric Diagnostics for Ultrashort Pulses

High-resolution Interferometric Diagnostics for Ultrashort Pulses

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3. PHASE RECONSTRUCTION ALGORITHM FOR MULTIPLE SPECTRAL SHEARINGINTERFEROMETRY32|βk ,m |10−0.4 −0.2 0 0.2 0.4t m /TFigure 3.5: (Color online) Modulus of the reconstruction coefficient |β k ,m | (eq. (3.31) in the text)<strong>for</strong> a single shear of Ω = 2π/T (solid blue) and <strong>for</strong> multi-shear retrieval with Ω 1 = Ω (dashed, red)and Ω 2 = 5Ω (dotted, green).gives further insight into the algorithm. The modulus of this factor is shown in Fig. 3.5 <strong>for</strong> the twoshearcase Ω 1 = Ω and Ω 2 = 5Ω, and compared with the single shear case. The larger shear (dottedgreen) in<strong>for</strong>mation is preferred at around t = 0 which corresponds to large scale spectral features.However, at t = ±T /5,±2T /5, the contribution from the larger shear drops to zero because itcontains no in<strong>for</strong>mation with this periodicity, and all in<strong>for</strong>mation is obtained from the smallershear, so that its coefficient equals the single-shear case at these points.To evaluate the overall per<strong>for</strong>mance, one considers ˜Γ k ,m to be corrupted by uni<strong>for</strong>m noise withunit variance. In the retrieval, the noise, along with the signal, is multiplied by (3.31), so that thetotal noise energy in { ˜φ m }, and equivalently in {φ n }, can be calculated by taking the Pythagoreansum of β k ,m over all shears and points in the quasi-time domainA 2 [{Ω k }]= 1 N−14Tm =1k e−it m Ω k − 1 2k (1 − cost m Ω k ) 2(3.32)One can compare the multiple shear case with simply taking the same number of measurementswith the same shear to obtain a “noise suppression factor”A[Ω] MS =. (3.33)A[{Ω k = Ω}] α SNR84

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