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PLANAR LIQUID SHEETS AT LOW REYNOLDS NUMBERS
Author(s) -
RAMOS J. I.
Publication year - 1996
Publication title -
international journal for numerical methods in fluids
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.938
H-Index - 112
eISSN - 1097-0363
pISSN - 0271-2091
DOI - 10.1002/(sici)1097-0363(19960530)22:10<961::aid-fld389>3.0.co;2-d
Subject(s) - reynolds number , curvature , mechanics , froude number , magnetic reynolds number , mathematics , geometry , physics , flow (mathematics) , turbulence
Asymptotic methods are employed to derive the leading‐order equations which govern the fluid dynamics of time‐dependent, incompressible, planar liquid sheets at low Reynolds numbers using as small parameter the slenderness ratio. Analytical and numerical solutions of relevance to both steady film casting processes and plane stagnation flows are obtained with the leading‐order equations. It is shown that for steady film casting processes the model which accounts for both gravity and low‐Reynolds‐number effects predicts thicker and slower planar liquid sheets than those which neglect a surface curvature term or assume that Reynolds number is zero, because the neglect of the curvature term and the assumption of zero Reynolds number are not justified at high take‐up velocities owing to the large velocity gradients that occur at the take‐up point. It is also shown that for Reynolds number/Froude number ratios larger than one, models which neglect the surface curvature or assume a zero Reynolds number predict velocity profiles which are either concave or exhibit an inflection point, whereas the model which accounts for both curvature and low‐Reynolds‐number effects predicts convex velocity profiles. For plane stagnation flows it is shown that models which account for both low‐Reynolds‐number and curvature effects predict nearly identical results to those of models which assume zero Reynolds number. These two models also predict a faster thickening of the planar liquid sheet than models which account for low‐ Reynolds‐number effects but neglect the surface curvature. This curvature term is very large near the stagnation point and cannot be neglected there. It is also shown that the thickening of the sheet occurs closer to the stagnation point as the Reynolds number/Froude number ratio is increased, i.e. as the magnitude of the gravitational acceleration is increased. In addition it is shown that large surface tension introduces a third‐order spatial derivative in the axial momentum equation at leading order.