200 research outputs found
Instability driven by boundary inflow across shear: a way to circumvent Rayleigh's stability criterion in accretion disks?
We investigate the 2D instability recently discussed by Gallet et al. (2010)
and Ilin \& Morgulis (2013) which arises when a radial crossflow is imposed on
a centrifugally-stable swirling flow. By finding a simpler rectilinear example
of the instability - a sheared half plane, the minimal ingredients for the
instability are identified and the destabilizing/stabilizing effect of
inflow/outflow boundaries clarified. The instability - christened `boundary
inflow instability' here - is of critical layer type where this layer is either
at the inflow wall and the growth rate is (as found by Ilin \&
Morgulis 2013), or in the interior of the flow and the growth rate is where measures the (small) inflow-to-tangential-flow
ratio. The instability is robust to changes in the rotation profile even to
those which are very Rayleigh-stable and the addition of further physics such
as viscosity, 3-dimensionality and compressibility but is sensitive to the
boundary condition imposed on the tangential velocity field at the inflow
boundary. Providing the vorticity is not fixed at the inflow boundary, the
instability seems generic and operates by the inflow advecting vorticity
present at the boundary across the interior shear. Both the primary bifurcation
to 2D states and secondary bifurcations to 3D states are found to be
supercritical. Assuming an accretion flow driven by molecular viscosity only so
, the instability is not immediately relevant for accretion
disks since the critical threshold is and the inflow boundary
conditions are more likely to be stress-free than non-slip. However, the
analysis presented here does highlight the potential for mass entering a disk
to disrupt the orbiting flow if this mass flux possesses vorticity.Comment: 44 pages, 14 figure
Coherent structures in localised and global pipe turbulence
The recent discovery of unstable travelling waves (TWs) in pipe flow has been
hailed as a significant breakthrough with the hope that they populate the
turbulent attractor. We confirm the existence of coherent states with internal
fast and slow streaks commensurate in both structure and energy with known TWs
using numerical simulations in a long pipe. These only occur, however, within
less energetic regions of (localized) `puff' turbulence at low Reynolds numbers
(Re=2000-2400), and not at all in (homogeneous) `slug' turbulence at Re=2800.
This strongly suggests that all currently known TWs sit in an intermediate
region of phase space between the laminar and turbulent states rather than
being embedded within the turbulent attractor itself. New coherent fast streak
states with strongly decelerated cores appear to populate the turbulent
attractor instead.Comment: As accepted for PRL. 4 pages, 6 figures. Alterations to figs. 4,5.
Significant changes to tex
Spatiotemporal dynamics in 2D Kolmogorov flow over large domains
Kolmogorov flow in two dimensions - the two-dimensional Navier-Stokes
equations with a sinusoidal body force - is considered over extended periodic
domains to reveal localised spatiotemporal complexity. The flow response
mimicks the forcing at small forcing amplitudes but beyond a critical value
develops a long wavelength instability. The ensuing state is described by a
Cahn-Hilliard-type equation and as a result coarsening dynamics are observed
for random initial data. After further bifurcations, this regime gives way to
multiple attractors, some of which possess spatially-localised time dependence.
Co-existence of such attractors in a large domain gives rise to interesting
collisional dynamics which is captured by a system of 5 (1-space and 1-time)
PDEs based on a long wavelength limit. The coarsening regime reinstates itself
at yet higher forcing amplitudes in the sense that only longest-wavelength
solutions remain attractors. Eventually, there is one global longest-wavelength
attractor which possesses two localised chaotic regions - a kink and antikink -
which connect two steady one-dimensional flow regions of essentially half the
domain width each. The wealth of spatiotemporal complexity uncovered presents a
bountiful arena in which to study the existence of simple invariant localised
solutions which presumably underpin all of the observed behaviour
Reply to Comment on 'Critical behaviour in the relaminarization of localized turbulence in pipe flow'
This is a Reply to Comment arXiv:0707.2642 by Hof et al. on Letter
arXiv:physics/0608292 which was subsequently published in Phys Rev Lett, 98,
014501 (2007).
In our letter it was reported that in pipe flow the median time for
relaminarisation of localised turbulent disturbances closely follows the
scaling . This conclusion was based on data from
collections of 40 to 60 independent simulations at each of six different
Reynolds numbers, Re. In the Comment, Hof et al. estimate differently
for the point at lowest Re. Although this point is the most uncertain, it forms
the basis for their assertion that the data might then fit an exponential
scaling , for some constant A, supporting Hof et al.
(2006) Nature, 443, 59. The most certain point (at largest Re) does not fit
their conclusion and is rejected. We clarify why their argument for rejecting
this point is flawed. The median is estimated from the distribution of
observations, and it is shown that the correct part of the distribution is
used. The data is sufficiently well determined to show that the exponential
scaling cannot be fit to the data over this range of Re, whereas the fit is excellent, indicating critical behaviour and supporting
experiments by Peixinho & Mullin 2006.Comment: 1 page, 1 figur
Energy dissipation rate limits for flow through rough channels and tidal flow across topography
The bound derived in the submission (subsequently published in J. Fluid
Mechanics vol 808 p 562-575, 2016) with the above title is incorrect. This
corrigendum explains why and also why there can not be any quick fix.Comment: This is a corrigendum (to be published in J. Fluid Mechanics
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