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Most polarimetric data for asteroids have been obtained at λ = 0.518 μm, adapted from Zellner and Gradie (1976).
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The lowest surface roughness (Ra = 0.332 nm) were obtained at Λ of 20 nm.
The maximum hardness of 34.0 GPa, which was considerably higher than the rule-of-mixture hardness of the constituent layers, was obtained at Λ = 31.1 nm.
For each region, there exists a case for which no rate splitting determines the overall region, i.e., each achievable rate region is obtained at λ = 0 or λ = 1.
The λ max was obtained at wavelength of 289 nm.
The optimal clustering solution was obtained at POD = 0.0086 corresponding to k = 2 and λ = 0.1.
This range has been previously obtained at λ = 633 nm for laser-irradiated carbon films with a large amount of graphite phase and dominating sp2-type bonds[21].
Compared to a standard Savonius turbine, a relative increase of the power output coefficient by almost 40% is finally obtained at λ = 0.7.
The lower residual stress (− 1.02 GPa) and the highest critical fracture load (Lmax = 68.8 mN) were also obtained at Λ = 40 nm.
The optimal pathway is obtained for λ = 0.9.
The highest AvgSn of 0.851 is obtained for λ = 5.
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