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The results present the different scattered field of the guided waves at the joint as a function of frequency, mode, excitation angle and presence of artificial damage.
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The ESPRIT algorithm with phase mode excitation is derived to estimate the 3D angles.
Since the IP shock discussed here has very similar properties to the one simulated by Oliveira and Raeder (2014), with exactly the same shock impact angle, their conclusions support the argument of the lack of cavity mode excitation in observed in the event discussed in this paper.
These authors concluded that the shock impact angle plays a major role in effectively compressing the magnetosphere, thereby leading to a more favorable scenario for cavity mode excitation due to symmetric magnetosphere compression.
We consider the cases of single mode excitation and simultaneous double mode excitation.
Mode excitation factors and mode phases analysis allow, respectively, localization in depth and distance.
(a) represents the mode excitation factor modulus (no sign information) and (b) shows the mode excitation factor modulus combined with sign information.
After modal filtering, the mode excitation factor modulus of each mode is calculated as a mean over the region.
The amplitude of the transform for each curve (dispersive mode) depends only on the mode excitation factor modulus.
The combination of mode excitation factors with mode signs allows canceling secondary peaks in the correlation function.
We demonstrate that adding the mode signs to the mode excitation factor modulus improves significantly the localization performance in depth.
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