Permeability sets the linear path instability of buoyancy-driven disks
نویسندگان
چکیده
The prediction of trajectories buoyancy-driven objects immersed in a viscous fluid is key problem dynamics. Simple-shaped objects, such as disks, present great variety trajectories, ranging from zig-zag to tumbling and chaotic motions. Yet, similar studies are lacking when the object permeable. We perform linear stability analysis steady vertical path thin permeable disk, whose flow through microstructure modelled via stress-jump model based on homogenization theory. relative velocity associated with presents recirculation region detached body, which shrinks eventually disappears disk becomes more In analogy solid one non-oscillatory several oscillatory modes identified found destabilize fluid–solid coupled system away its straight trajectory. Permeability progressively filters out wake dynamics instability path. Modes dominated by oscillations first stabilized, followed those characterized weaker, or absent, oscillations, typically tilting induced inclined For sufficiently large permeabilities, undergoes divergence instability, expected lead oblique constant inclination, nonlinear regime. A further permeability increase reduces unstable range all until quenching instabilities.
منابع مشابه
on the effect of linear & non-linear texts on students comprehension and recalling
چکیده ندارد.
15 صفحه اولA Gravitational Instability-Driven Viscosity in Self-Gravitating Accretion Disks
We derive a viscosity from gravitational instability in self-gravitating accretion disks, which has the required properties to account for the observed fast formation of the first super-massive black holes in highly redshifted quasars and for the cosmological evolution of the black hole-mass distribution. Subject headings: accretion, accretion disks — hydrodynamics — turbulence — galaxies: acti...
متن کاملA Wind Driven Warping Instability in Accretion Disks
A wind passing over a surface may cause an instability in the surface such as the flapping seen when wind blows across a flag or waves when wind blows across water. We show that when a radially outflowing wind blows across a dense thin rotating disk, an initially flat disk is unstable to warping. When the wind is subsonic, the growth rate is dependent on the lift generated by the wind and the p...
متن کاملThe stability of protostellar disks with Hall effect and buoyancy
The stability properties of inviscid protostellar disks are examined taking into account the Hall effect and buoyancy. Depending on the parameters, different types of instabilities can exist in different regions of disks. In a very low ionized region, the instability associated with baroclinic effects of buoyancy is likely most efficient. The Hall-driven shear instability can lead to destabiliz...
متن کاملThe Stability of Buoyancy-driven Coastal Currents
Griffiths, R.W. and Linden, P.F., 1981. The stabil i ty of buoyancy-dr iven coastal currents. Dyn. Atmos . Oceans, 5: 281--306. Buoyancy-dr iven boundary currents were generated in the labora tory by releasing buoyan t fluid f rom a source adjacent to a vertical boundary in a rota t ing container . The boundary removed the Coriolis force parallel to it, a l lowing the buoyan t fluid to spread i...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of Fluid Mechanics
سال: 2023
ISSN: ['0022-1120', '1469-7645']
DOI: https://doi.org/10.1017/jfm.2022.989