Fig. 6.

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Detectability of the solar cycle in individual skip travel times. (A) Amplitudes of travel-time variations due to the solar cycle, As, versus skip number s (see Eq. (18)), with error bars of (see Eq. (19)). (B) Signal-to-noise ratios
. (C) Variance of travel-time noise
. (D) Plot of Λs, s′ = 19 and (E) plot of Rs, s′ = 19. In all panels, the blue and red points show the even and odd values of s.
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