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NASA NTRS ยท 19810013781

Instability and transition in rotating disk flow

Abstract

The stability of three dimensional rotating disk flow and the effects of Coriolis forces and streamline curvature were investigated. It was shown that this analysis gives better growth rates than Orr-Sommerfeld equation. Results support the numerical prediction that the number of stationary vortices varies directly with the Reynolds number.

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BibTeXRIS

Malik, M. R.. 1981-03-01. Instability and transition in rotating disk flow. https://ntrs.nasa.gov/citations/19810013781

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