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In order to ensure correct communication of solutions on the interfaces of grids with different time step sizes, the values at intermediate-stages of the Runge Kutta time integration on the elements neighboring such interfaces are coupled with minimal dissipation and dispersion errors.
For both parameters and for all cluster sizes, the values are normalized by the control case (n = 1).
Regarding the trend of our data in Fig. 4a, over a wide range of peak energies (QD sizes) the values of the FSS are nearly constant.
We also note that at smaller sizes, the values of the RSM were more constrained, while at larger sizes there was more variation, i.e., at large size different wing shapes were observed.
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2. Sizing the value constellation.
For determination of the magnitude of effect sizes the following values were used.
Due to the large sample sizes the critical p-value was set at p = .01.01
We also found that at small size, the values of the RSM were more constrained than at large size.
Bubble sizes are the values in a unit of SD deviated from the central control line.
For the former setting the similarity across K-values has obviously increased, while at the same time the sizes of the values have not decreased strongly.
If we compacting overall volume size, the value of spherical aberration (SA) at wide radius of contact lens seems lower.
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