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W805496018 abstract "Recent theoretical studies by Lingwood (1995,1997a,b) on the rotating-disk boundary-layer, have shown, using an analysis that deploys the usual 'parallel-flow' approximation, that there exists a region of absolute instability. However, by taking into account the radial variation of the mean flow, Davies h Carpenter (2003) have shown, using numerical simulations, that the absolute instability does not give rise to an unstable linear global mode. In fact convective behaviour is found to dominate the global response. The aim of the current study is to further the studies of Davies h Carpenter (2003) to other rotating boundary-layers. Uniform suction and a uniform axial magnetic field are known to be stabilizing. However, by considering non-parallel effects, globally unstable behaviour is observed, albeit without the promotion of a fixed global frequency. An investigation is also carried out on the so called BEK family of rotating boundary-layers, which includes the Bodewadt, Ekman and von Karman flows. All of these flows are absolutely unstable, when the parallel flow approximation is applied. However, by considering the genuine non-parallel flow, the numerical simulation results indicate that the kind of behaviour found for the von Karman flow is carried over to other flows in the BEK family. The numerical simulation results of the rotating-disk boundary-layer can be modeled using the linearized complex Ginzburg-Landau equation. By deriving expressions for the stability, convection velocity and diffusion/dispersion effects, in terms of the numerical simulation results, the Green's solutions to the Ginzburg-Landau equation can be successfully matched to the parallel and non-parallel rotating-disk boundary-layer. The results suggest that the long-term behaviour depends on the precise balance of the varying frequency, varying growth rate, and diffusion/dispersion effects. It is then possible for an absolutely unstable disturbance to remain globally stable." @default.
W805496018 created "2016-06-24" @default.
W805496018 creator A5002177029 @default.
W805496018 date "2007-01-01" @default.
W805496018 modified "2023-09-25" @default.
W805496018 title "Numerical simulations of disturbance development in rotating boundary-layers" @default.
W805496018 cites W1510620470 @default.
W805496018 cites W1587415653 @default.
W805496018 cites W1614849757 @default.
W805496018 cites W1621729193 @default.
W805496018 cites W1633953027 @default.
W805496018 cites W1647852048 @default.
W805496018 cites W182983404 @default.
W805496018 cites W1964799215 @default.
W805496018 cites W1966011892 @default.
W805496018 cites W1967036484 @default.
W805496018 cites W1967694768 @default.
W805496018 cites W1973944475 @default.
W805496018 cites W1974485540 @default.
W805496018 cites W1974490836 @default.
W805496018 cites W1977268243 @default.
W805496018 cites W1980200814 @default.
W805496018 cites W1981777274 @default.
W805496018 cites W1987380113 @default.
W805496018 cites W1988938197 @default.
W805496018 cites W1990431093 @default.
W805496018 cites W1990946432 @default.
W805496018 cites W1991261345 @default.
W805496018 cites W1992173980 @default.
W805496018 cites W1996993815 @default.
W805496018 cites W2001014984 @default.
W805496018 cites W2004121879 @default.
W805496018 cites W2007932842 @default.
W805496018 cites W2009249898 @default.
W805496018 cites W2018200376 @default.
W805496018 cites W2019545630 @default.
W805496018 cites W2021200189 @default.
W805496018 cites W2024023202 @default.
W805496018 cites W2029854885 @default.
W805496018 cites W2036199851 @default.
W805496018 cites W2036392167 @default.
W805496018 cites W2037260346 @default.
W805496018 cites W2038383239 @default.
W805496018 cites W2038776074 @default.
W805496018 cites W2040842965 @default.
W805496018 cites W2041117630 @default.
W805496018 cites W2041772700 @default.
W805496018 cites W2042251803 @default.
W805496018 cites W2042751607 @default.
W805496018 cites W2043995567 @default.
W805496018 cites W2044337541 @default.
W805496018 cites W2046759584 @default.
W805496018 cites W2046935531 @default.
W805496018 cites W2049322015 @default.
W805496018 cites W2049662547 @default.
W805496018 cites W2051722940 @default.
W805496018 cites W2057020942 @default.
W805496018 cites W2057970519 @default.
W805496018 cites W2058987288 @default.
W805496018 cites W2059274336 @default.
W805496018 cites W2059519139 @default.
W805496018 cites W2059724153 @default.
W805496018 cites W2062349631 @default.
W805496018 cites W2063018965 @default.
W805496018 cites W2063377918 @default.
W805496018 cites W2066035123 @default.
W805496018 cites W2069103814 @default.
W805496018 cites W2071396303 @default.
W805496018 cites W2074000879 @default.
W805496018 cites W2076579506 @default.
W805496018 cites W2079469401 @default.
W805496018 cites W2079863474 @default.
W805496018 cites W2080538334 @default.
W805496018 cites W2082585590 @default.
W805496018 cites W2084517518 @default.
W805496018 cites W2086656011 @default.
W805496018 cites W2087296376 @default.
W805496018 cites W2089073422 @default.
W805496018 cites W2089648411 @default.
W805496018 cites W2095867813 @default.
W805496018 cites W2100975431 @default.
W805496018 cites W2101485529 @default.
W805496018 cites W2104102786 @default.
W805496018 cites W2104334205 @default.
W805496018 cites W2104852085 @default.
W805496018 cites W2104860737 @default.
W805496018 cites W2115919469 @default.
W805496018 cites W2118495386 @default.
W805496018 cites W2125692555 @default.
W805496018 cites W2129661721 @default.
W805496018 cites W2131273370 @default.
W805496018 cites W2137517745 @default.
W805496018 cites W2145964070 @default.
W805496018 cites W2146344841 @default.
W805496018 cites W2147920701 @default.
W805496018 cites W2153511311 @default.
W805496018 cites W2155450104 @default.
W805496018 cites W2158683843 @default.
W805496018 cites W2162890609 @default.
W805496018 cites W2163807646 @default.