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contributor authorRoger E. Khayat
date accessioned2017-05-09T00:28:25Z
date available2017-05-09T00:28:25Z
date copyrightJune, 2008
date issued2008
identifier issn0098-2202
identifier otherJFEGA4-27318#061202_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/138216
description abstractSteady two-dimensional thin-film flow of a Newtonian fluid is examined in this theoretical study. The influence of exit conditions and gravity is examined in detail. The considered flow is of moderately high inertia. The flow is dictated by the thin-film equations of boundary layer type, which are solved by expanding the flow field in orthonormal modes in the transverse direction and using Galerkin projection method, combined with integration along the flow direction. Three types of exit conditions are investigated, namely, parabolic, semiparabolic, and uniform flow. It is found that the type of exit conditions has a significant effect on the development of the free surface and flow field near the exit. While for the parabolic velocity profile at the exit, the free surface exhibits a local depression, for semiparabolic and uniform velocity profiles, the height of the film increases monotonically with streamwise position. In order to examine the influence of gravity, the flow is studied down a vertical wall as well as over a horizontal wall. The role of gravity is different for the two types of wall orientation. It is found that for the horizontal wall, a hydraulic-jump-like structure is formed and the flow further downstream exhibits a shock. The influence of exit conditions on shock formation is examined in detail.
publisherThe American Society of Mechanical Engineers (ASME)
titleInfluence of Upstream Conditions and Gravity on Highly Inertial Thin-Film Flow
typeJournal Paper
journal volume130
journal issue6
journal titleJournal of Fluids Engineering
identifier doi10.1115/1.2928387
journal fristpage61202
identifier eissn1528-901X
treeJournal of Fluids Engineering:;2008:;volume( 130 ):;issue: 006
contenttypeFulltext


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