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The boundary layer saturation is Eq. 18.

S b = ∑ r min r max h i r i 2 · α i, (18 where Sb is boundary layer saturation, dimensionless; rmin is the minimal throat radius, μm; rmax is the maximal throat radius, μm; h i is boundary layer thickness in the throat whose radius is r i, μm; α i is proportion of throats whose radius is r i, dimensionless.

The upper boundary of IIP3 saturation is related to thermal noise.

Oil saturation and water saturation in boundary layer is calculated according to Eqs.

To improve the chattering induced by the traditional sliding mode control and guarantee the reachability of the system, a specific saturation function with dynamic boundary layer is proposed to replace the sign function in the preceding control law.

The top of the daytime boundary layer is referred to as the mixed-layer inversion.

The fluid in the boundary layer is subjected to shearing forces.

The region above the planetary boundary layer is commonly known as the free atmosphere.

This boundary layer is approximately 0.3 nm thick.

The region outside the boundary layer is characterized by substantial mixing or turbulence.

A boundary layer flow was indirectly detected.