Deterministic and stochastic aspects of the transition to turbulence
Deterministic and stochastic aspects of the transition to turbulence
Baofang Song and Björn Hof
IST Austria (Institute of Science and Technology Austria), 3400 Klosterneuburg, Austria
Max Planck Institute for Dynamics and Self-Organization, Bunsenstrasse 10, Göttingen, Germany
The purpose of this contribution is to summarize and discuss
recent advances regarding the onset of turbulence in shear flows.
The absence of a clear cut instability mechanism, the spatio-temporal
intermittent character and extremely long lived transients
are some of the major difficulties encountered in these flows and
have hindered progress towards understanding the transition process.
We will show for the case of pipe flow that concepts from nonlinear dynamics and statistical
physics can help to explain the onset of turbulence. In particular
the turbulent structures (’puffs’) observed close to onset are
spatially localized chaotic transients and their lifetimes increase
super exponentially with Reynolds number. At the same time
fluctuations of individual turbulent puffs can (although very rarely)
lead to the nucleation of new puffs. The competition between these
two stochastic processes gives rise to a non-equilibrium phase
transition where turbulence changes from a super-transient to a
How turbulence first arises in simple shear flows has remained
an open question for well over a century. Osborne Reynolds  was
the first to observe that this transition depends on a dimensionless
group, i.e. the Reynolds number, as well as on the amplitude of
disturbances present in the system. Some of the leading theorists
at the time (e.g. Lord Kelvin, Lord Rayleigh, Arnold Sommerfeld,
Werner Heisenberg, Hendrik Antoon Lorentz ) attempted to probe the stability of pipe and
related shear flows (i.e. channel and Couette flow) with essentially
linear methods. After many unsuccessful attempts it has
become clear (e.g. see ) that the occurrence of
turbulence is unrelated to the stability of the laminar state, as
Reynolds had already concluded from his experimental observations
many years earlier. While pipe and Couette flow are believed to
be stable for all Reynolds numbers, plane Poiseuille (i.e. channel)
flow becomes unstable at Re of about 5800. However in the latter
case turbulence is typically already observed at Reynolds numbers
a little above 1000 and to hold the flow laminar up to the linear
stability threshold actually requires considerable effort in experiments.
Transition in the type of flows discussed above is qualitatively different from the classical pictures for the transition to turbulence which goes back to Landau and to Ruelle and Takens . In both scenarios turbulence arises following a sequence of instabilities of the base flow (which hence becomes linearly unstable). While the Ruelle Takens type transition has been observed in several closed flows (e.g. ) it is noteworthy that even in this case the transition sequence only explains the onset of comparably low dimensional chaotic motion which dynamically is still far from the full spatio-temporal complexity encountered in turbulent flows. In open shear flows such as pipes all experimental observations show that the transition in contrast is rather abrupt directly from laminar to turbulent. The latter type of transition has turned out to be far more difficult to understand.
In more recent years a new transition mechanism has been proposed based on dynamical systems concepts. Invariant solutions of the Navier Stokes equations such as periodic orbits or traveling waves are deemed to be ultimately responsible for the existence of the turbulent state. These new solutions
In pipe flow turbulent puffs (Fig. 1(top)) are typically observed in a
Reynolds number regime of approximately .
They result from perturbations of finite amplitude and in experiments if
no great care is taken they will often result from distortions the
flow experiences directly at the inlet. If the inlet is designed
carefully to avoid such disturbances and if the pipe is sufficiently straight and smooth, flows can be held laminar up
to much higher ( the record in experiments is currently at =100000).
For controlled studies of transition it is desirable to start with a
laminar flow and to study its response to a well controlled disturbance
which for example can be a jet of fluid injected for a brief period
through a small hole in the pipe wall. If the amplitude of such a
perturbation is large enough a turbulent puff is created. While directly
after the flow has been perturbed the dynamics depend on the nature of the
disturbance (the puff first has to develop), after 100 to 150 advective time units (measured in D/U, where D is the diameter and U the mean velocity) the resulting puff is independent of the perturbation that
Curiously in this Reynolds number regime turbulence always remains localized. Even if an extended (axially) part of the pipe is disturbed the flow will always arrange itself in turbulent segments (i.e. puffs) which are about to long (the turbulent core excluding the leading edge) and interspersed by laminar fluid. Vorticity isosurfaces of a turbulent puff at are shown in Fig. 1(top). Fig. 1(bottom) shows energy levels in a space time plot (time from bottom to top) of a simulation of an initially (t=0) fully turbulent flow. Upon reduction of to 2200 laminar regions (blue) appear and turbulence becomes confined to localized regions, i.e. puffs (red vertical stripes in Fig. 1(bottom)). The direct numerical simulations were carried out with a spectral code . Fourier modes in the axial and azimuthal direction and finite difference in the radial are employed and the resolution chosen here is in radial, axial, and azimuthal directions. The domain is in the axial direction ( being the diameter) with periodic boundary conditions.
As pointed out in
 at Reynolds numbers close to 2000
turbulent puffs extract energy from the adjacent (actually upstream)
laminar parabolic flow. The plug like turbulent profile in the central
part of the puff is unable to sustain turbulence (or rather to feed
turbulence in the downstream direction) consequently the turbulence
intensity decreases along the leading edge of the puff in the
downstream direction and the flow eventually relaminarises. Due to
the action of viscosity the laminar profile now begins to recover
its parabolic shape so that at sufficient distance a second puff
can be sustained. If on the other hand the distance between puffs
is too short the downstream puff will border onto fluid with a flatter
plug like profile in the upstream direction. Consequently it cannot extract sufficient kinetic
energy from the flow upstream and decays as shown in
. The interaction distance between two puffs is approximately
. As a result turbulent puffs have a minimum spacing
of that same distance. While this argument qualitatively explains
why fully turbulent flow cannot be sustained at these low Re, the
energetic aspects of this process are not understood in full detail.
A key attribute of puffs is their highly chaotic dynamics. This gives rise to a loss of memory and limits the prediction of the flows future evolution. To illustrate the sensitive dependence on initial conditions we simulated two puffs with velocity fields that only deviate by . As usual for chaotic systems this deviation grows exponentially and as can be seen form the energy time series shown in Fig. 2 the signals notably depart and become completely unrelated after about 200 advective time units (the time the puffs takes to travel 200 pipe diameters downstream). The loss of predictabiliy becomes especially clear when one puff suddenly decays (green curve in Fig. 2) while the other continues unchanged (i.e. the average quantities remain unchanged).
It is a typical feature of puffs that they live for very long times and decay suddenly (see Fig. 2). Extensive statistical studies have shown that the survival probability is exponentially distributed and the decay is memoryless. This behaviour is in line with the escape from chaotic repellers observed in lower dimensional systems [20, 21]. Here a chaotic attractor turns into a chaotic saddle after an unstable periodic orbit within the attractor and one on the basin boundary collide (unstable-unstable pair bifurcation). Above the bifurcation point chaotic transients persist for very long times before they eventually decay.
A similar scenario has recently been observed for pipe flow. In this numerical study the dynamics were confined to a symmetry subspace (imposing a mirror and a 2-fold rotation symmetry with respect to the pipe axis). While this somewhat simplifies the dynamics the flow still exhibits turbulent motion for large enough Re. By following the laminar turbulent boundary (the so called âedge stateâ , which in this case is a localised periodic orbit) to lower Re the saddle node bifurcation where the periodic orbits originates was reached (at =1430). The upper branch of this saddle node however is a stable periodic orbit(see Fig. 4) and again localised and its length is comparable to that of puffs.
For increasing Re the orbit
first undergoes a secondary Hopf bifurcation followed by the formation
of a chaotic attractor. This is the point where chaotic motion originates
in this subspace. The basin of the attractor increases rapidly
with until it reconnects with the unstable periodic orbit on the
basin boundary. At this moment the chaotic dynamics turn into long
lived transients (presumably following an unstable-unstable pair bifurcation).
The memoryless nature of the decay and the loss of predictability is a
direct consequence of the sensitive dependence on initial conditions
characteristic for deterministic chaos.
While the classical picture of turbulence is that of a chaotic attractor, dating back to the landmark paper of Ruelle and Takens, this approach only takes the temporal dynamics into account and neglects the spatial complexity which is however intrinsic to turbulent flows. The importance of spatial aspects and the spatio temporal intermittent character of the turbulence transition have been emphasized in studies of model system [17, 19]. Also the chaotic attractor hypothesis has been questioned in 1980’s by Crutchfield and Kaneko  who propose that chaotic super transients are more relevant to turbulence. A first observation supporting this view came from direct numerical simulations of pipe flows where transients were observed . A number of later studies were concerned with long lived transients at low Reynolds numbers in pipe flow [23, 24, 25, 26, 27, 28, 29] and found that the decay is a memoryless process with a characteristic lifetime which is a function of Re. There was however no consensus if or if not the lifetimes of individual puffs became infinite or remained finite. A number of studies proposed that the turbulent flow decay rates (inverse characteristic lifetimes) scale as [13, 23, 24] or at least as a power law . This view was questioned by Hof  who found that instead implying that turbulence remains transient. In a refined study for much longer observation times than in any previous study (spanning almost 8 orders of magnitude in time) was found to scale super exponentially with 
A more direct analogy can be drawn
to another model system of coupled chaotic maps which is motivated by
bistable excitable media . A key difference to the above mentioned map models is that here
the susceptibility of a âlaminarâ site to perturbations
from neighbouring chaotic sites (and hence the minimum perturbation
amplitude to trigger chaotic dynamics at a laminar site), decreases
with (where is a the control parameter analogous to the Reynolds number).
This model input reflects experimental observations of pipe flow where
the minimum perturbation amplitude to trigger turbulence was found to
scale with [32, 9, 33].
In the model just like in the experiments localized excited states,
i.e. puffs, with transient lifetimes are observed and with an increase in
the control parameter lifetimes of individual puffs scale faster than
exponential and hence remain transient.
Consequently in pipe flow the increase in the temporal complexity alone does not lead to sustained turbulence. As proposed by Moxey and Barkley  and later explicitly shown by Avila et al.  turbulence becomes sustained by a spatial growth process called puff splitting. Puff splitting is commonly observed at Reynolds numbers of around 2300 [36, 37] and while here turbulence is still confined to puffs typically to in length puff sizes fluctuate and can occasionally reach larger values. In these instances in a small number of cases a segment of turbulent fluid at the leading edge of the puff can escape further downstream beyond the puff-puff interaction distance and a new puff develops here (see Fig. 4). This splitting process leads to an increase in turbulent fraction.
As shown by Avila et al. 
puff splitting is also intrinsically memoryless and can already be
found at much lower Re as previously expected. The characteristic time
for such an event to occur decreases super-exponentially with Re.
The argument for turbulence to become sustained is now straightforward.
If the characteristic time for turbulent puffs to decay is smaller
than the time for new puffs to be created (i.e. by splitting) turbulence will
eventually decay. If on the other hand new puffs are created faster
than existing ones decay in the thermodynamic limit turbulence becomes
sustained. The critical Reynolds number where turbulence changes from
a transient to a sustained state can be estimated by the intersection
point of the characteristic time scales of the two processes shown in
This transition is analogous to non equilibrium phase transitions and as we will argue below, bears close resemblance to directed percolation (DP) and related contact processes. First speculations about a possible connection between transition in linearly stable shear flows and DP date back to Pomeau in 1986 . Just like in DP, pipe flow has a unique absorbing state which is the laminar flow. Once turbulence has decayed the flow cannot by itself return to turbulence unless it is disturbed from the outside. The recent studies of puff decay and splitting [27, 35] also suggest that the interaction is only short range, which is another requirement for DP . No observations indicate that a localized puff would create a second one in a part of the pipe not adjacent to it (i.e. more than 25 D or so away). Equally it has never been observed that puffs would influence the lifetimes of other puffs that are sufficiently far away. These recent studies also infer that if such a realtion to DP exists a single unit (i.e. a lattice point in DP) must correspond to a turbulent puff and not for example to a single vortex. To explore this analogy further hence requires much larger system sizes allowing to follow the evolution of many turbulent puffs(/spots). While a number of earlier studies (e.g. ) looked at such aspects retrospectively the system sizes used were too small.
In a numerical investigation  of plane Couette we consequently
chose a narrow but very long domain so that a large
number of turbulent stripes (analogous structure to puffs in pipes)
could be accommodated. This study gave more direct evidence that
the transition is indeed a non-equilibrium continuous phase transition.
Here just like in pipe flow super-exponential lifetime and splitting
statistics were observed for single stripes, and a critical point for the onset of
sustained turbulence could be determined in the same manner described above.
The much shorter time scales at the intersection point between
decay and splitting curves allowed to resolve size distributions
at this point. The distributions of laminar gaps exhibit scale
invariance supporting the proposition of a continuous phase transition.
Also here the same transition scenario between transient localized
chaos and sustained spatio temporal intermittent chaos was found.
Analogies to DP have also been explored in recent theoretical studies, e.g. [31, 42, 43] In particular for the coupled map model presented in  close agreement was found to the experimental results for pipe flow: the turbulent state becomes sustained when the splitting outweighs the decay of individual puffs. In addition the critical exponent for the increase of the turbulent fraction above onset was found to agree well with the universal one for DP in dimension.
While at present a final answer to the question if the laminar turbulence transition is a non-equilibrium phase transition in accordance with DP is outstanding experiments and numerical simulations to clarify this question are under way. One of the main challenges here is to resolve the extremely long time scales relevant in the vicinity of the transition point (note that characteristic splitting and decay times in pipes correspond to almost advective time units!). In this time puffs trave a distance correpsonding to pipe diameters. Equally an accuracy in the Reynolds number of about 0.1% is required setting a further challenge for experiments. A further open issue is the transition from spatially intermittent turbulence (i.e. puffs) to expanding space filling turbulent structures which takes place somewhere between Reynolds numbers 2300 and 3000.
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