NASA NTRS · 19900051617
Secondary instability in rotating disk flow
Abstract
Primary instability of the three-dimensional boundary layer on a rotating disk introduces periodic modulation of the mean flow in the form of cross-flow vortices. The stability of this modulated base flow to secondary disturbances is studied. In a three-dimensional boundary layer the threshold primary amplitude for secondary instability is larger than that for a two-dimensional boundary layer. The secondary instability results in a pair of traveling counter-rotating vortices, tilted up and oriented at an angle to the primary cross-flow vortices.
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Balachandar, S., Malik, M. R., Streett, C. L.. 1990-06-01. Secondary instability in rotating disk flow. https://ntrs.nasa.gov/citations/19900051617
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