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Earth, Planets and Space
Fig. 8 | Earth, Planets and Space

Fig. 8

From: Array-size dependency of the upper limit wavelength normalized by array radius for the standard spatial autocorrelation method

Fig. 8

Comparison between the reference model (black lines) and the observed phase velocities of each array (colored marks). The thin curves along with the model curve represent the ± 20% discrepancies from the model. Observed dispersion curves are plotted only partially in a wavelength range from 2.4r to 2.8r. The figures in the legend indicate the array radii

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