Helioseismological determination of the subsurface spatial spectrum of solar convection: Demonstration using numerical simulations

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Fig. 2.

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Example noiseless travel times τ_NR (bottom left panel) corresponding to the right panel in Fig. 3 and contributions from the different flow components (top panels) as well as different depth ranges (remaining panels) obtained using Eq. (2) with ϵ = 0.

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