1984
DOI: 10.1007/bf00905629
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Spatial stability of a liquid film on a rotating disk

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Cited by 3 publications
(3 citation statements)
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“…They found that axisymmetric perturbations have the largest amplification factors and Coriolis forces exert a stabilizing influence. Eliseev (1983), who examined the linear stability of timeperiodic perturbations, showed that the wavelength of the perturbation determines the radial domain of the instability, which becomes wider with increasing wavelength. The range of unstable wavenumbers approaches that for the falling film case with increasing radius.…”
Section: Introductionmentioning
confidence: 99%
“…They found that axisymmetric perturbations have the largest amplification factors and Coriolis forces exert a stabilizing influence. Eliseev (1983), who examined the linear stability of timeperiodic perturbations, showed that the wavelength of the perturbation determines the radial domain of the instability, which becomes wider with increasing wavelength. The range of unstable wavenumbers approaches that for the falling film case with increasing radius.…”
Section: Introductionmentioning
confidence: 99%
“…perturbations have the largest growth rates; they also found Coriolis forces to be stabilizing. Eliseev (1983) showed that the width of the linear instability domain increases with wavelength for time-periodic disturbances and approaches that for falling fi lms with increasing radius. Sisoev and Shkadov (1987) considered the limit of large E and examined the linear stability of axisymmetric perturbations for locally uniform fl ow.…”
Section: Steady Solutions Linear Stability and Lubrication Theorymentioning
confidence: 99%
“…Steady flow in the frame of the boundary layer approximation was considered by Dorfman12 and Sisoev et al ,13 where transitions from arbitrary inlet film flow to the Nusselt solution were computed. Analysis of the linear stability of the steady axisymmetric flow was performed using asymptotic methods2, 5, 11, 14 and the full Navier–Stokes equation for finite Eckman numbers 15. 16 The simplest non‐linear evolution equations based on the lubrication approximation for radial velocity were discussed by Emslie et al 17 and recently by Momoniat and Mason,18 where additional references may be found.…”
Section: Introductionmentioning
confidence: 99%