Fig. 3

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Normalized integral dependence on distance d to the turbulent phase screen for CSD if the VLT design is with (solid lines) or without a secondary mirror (dashed lines). Integral
averaged over all P-stars (different type symbols for each k mode shown) within a sky field No. 12. Integral
for each P-star in those fields (gray symbols, k = 6 only). Integrals were computed for R = 2.1′.
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