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Regional density of WMNs in sulcal depths and gyral crowns. All four regions showed significantly greater WMN density in the gyral crown compared to the sulcal depth (*p < 0.05). Across the four regions, both sulcal and gyral WMN density was least for cingulate (Cing)/SFG and greatest for the TE region. Temporal and parietal (Par) regional counts were significantly greater than counts for Cing/SFG (#p < 0.05).
