Search NASA⌕ Search

NASA NTRS · 19830043197

Numerical solutions for spin-up from rest in a cylinder

Abstract

A set of three-dimensional flow-field data for the region around a cylinder impulsively spun-up from rest was derived with a numerical model based on the Navier-Stokes equations. Laser-Doppler anemometer data in the azimuthal direction was employed to test the model predictions, and data was developed for a flowfield with Ekman numbers from 9.18/1,000,000 to 9.18/10,000. The contributions of inviscid and viscous terms were determined as functions of radius and time. It was found that immediately after start-up viscous diffusion is the dominant factor, which is replaced by nonlinear radial advection. The Coriolis force dominates in the later stages of spin-up. The inward radial flow is a maximum near the front, where the vertical velocity is small, but features strong radial gradients, as it does at the edge of the Ekman layer.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Hyun, J. M., Leslie, F., Fowlis, W. W., Warn-Varnas, A.. 1983-02-01. Numerical solutions for spin-up from rest in a cylinder. https://ntrs.nasa.gov/citations/19830043197

Cite the original work for its findings. Save a collection to share your selection of sources.