A Model of a Turbulent Boundary Layer With a Non-Zero Pressure Gradient
Abstract
According to a model of the turbulent boundary layer proposed by the authors, in the absence of external turbulence the intermediate region between the viscous sublayer and the external flow consists of two sharply separated self-similar structures. The velocity distribution in these structures is described by two different scaling laws. The mean velocity u in the region adjacent to the viscous sublayer is described by the previously obtained Reynolds-number-dependent scaling law ϕ= u/u*=Aηα, A=13 ReΛ+ 52, α=32 ReΛ, η= u* y/ν. (Here u* is the dynamic or friction velocity, y is the distance from the wall, ν the kinematic viscosity of the fluid, and the Reynolds number ReΛ is well defined by the data) In the region adjacent to the external flow the scaling law is different: ϕ= Bηβ. The power β for zero-pressure-gradient boundary layers was found by processing various experimental data and is close (with some scatter) to 0.2. We show here that for non-zero-pressure-gradient boundary layers, the power β is larger than 0.2 in the case of adverse pressure gradient and less than 0.2 for favourable pressure gradient. Similarity analysis suggests that both the coefficient B and the power β depend on ReΛ and on a new dimensionless parameter P proportional to the pressure gradient. Recent experimental data of Perry, Marušić and Jones (1)-(4) were analyzed and the results are in agreement with the model we propose.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.