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Rotationally symmetric fluctuating flow about a rotating disk

โœ Scribed by Arun Kumar Verma

Publisher
Elsevier Science
Year
1984
Tongue
English
Weight
560 KB
Volume
22
Category
Article
ISSN
0020-7225

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The perturbation equations which characterize the stability of flow over a rotating infinite disk are derived via strict order of magnitude analysis. These equations contain viscous terms not considered by Stuart,' curvature and Coriolis terms not considered by Brown? and axial velocity terms not co