This discrepancy results in increased levels of energy needing to be absorbed in larger scale sizes, leading to greater levels of impact damage in the larger scale sizes.
These wave structures have large-scale sizes compared to the finer structures of EPIs in the example as shown in Fig. 7, for example.
Nowadays, more and more attentions are paid to electromagnetic incremental forming (EMIF), especially for a part with a large-scale size, e.g., an integral panel with stiffened ribs.
Further study in a large scale sample size is needed.
Results from similar studies were considerably significant nonetheless, our study made use of a large scale population size.
The occurrence of larger zonal scale sizes during early evening hours is consistent with the results reported by Singh et al. (1997) based on measurements from a low-inclination satellite, AE-E.
From the Swarm spacecrafts with zonal separations of about 150 km, we conclude that larger zonal scale sizes of irregularities exist during the early evening hours (around 1900 LT).
This effect saturates for very small scaled population sizes, but diverges for very large scaled population sizes, to the point that reproductive isolation will take extremely long times for very large population sizes (4 N e κ F ≫ 10 ).
This explains the slowdown of the accumulation of DMIs for large scaled population sizes observed in Figure 1.
For large scaled population sizes, we see that distributions are peaked near the optimal binding strength Δ G = 0, reflecting the efficacy of selection in large populations.
As discussed above a major determinant at large scaled population sizes of the time for RI to develop is the rate of substitutions on each lineage, the inverse of which is plotted as a dashed line in Figure 4; we see that although the inverse substitution rate is a good predictor for large scaled population sizes, for small scaled populations it fails.
