In a combined experimental and direct-numerical study of the turbulent von Kármán flow (swirling flow between counter-rotating impellers), Faller and co-workers (J. Fluid Mech. 914, A2, 2021) showed that local interscale energy transfer and vorticity are both strongly intermittent and correlated, that the multifractal spectrum of the transfer field is milder than that of velocity or vorticity increments, and that the shear layer exhibits a highly correlated tail suggestive of self-similar quasi-singular structures reminiscent of Euler-equation singularities. They left four issues open: the causal direction between local energy transfer and vorticity intensification (their maxima are spatially displaced); whether the shear-layer vortices are self-similar quasi-singular structures that dominate high-order scaling; whether the milder transfer intermittency is a resolution artifact or a genuine physical distinction; and whether these properties are universal or specific to the von Kármán geometry. Recent work has made substantial partial progress — time-resolved 4D particle-tracking measurements of extreme transfer events by the same collaboration (2025), a contrasting null correlation in homogeneous isotropic turbulence (2023), perturbation-based causal analysis in isotropic turbulence (2023), and an active theory of strain self-amplification — but none of the four questions is settled; the problem remains open at its original generality.

Background

Turbulence intermittency denotes the concentration of small-scale turbulent activity — velocity gradients, dissipation, and inter-scale energy flux — into rare, violent, spatially clumped events, producing measurable deviations of structure-function scaling from Kolmogorov's 1941 self-similar theory (K41). A structure function Sp(ℓ)=⟨∣δuℓ∣p⟩S_p(\ell)=\langle|\delta u_\ell|^p\rangle averages the pp-th power of velocity increments over separations ℓ\ell; intermittency makes its scaling exponents depart from the K41 line ζp=p/3\zeta_p=p/3. In the multifractal framework, the set of points where increments scale as δuℓ∼ℓh\delta u_\ell\sim \ell^h has a fractal dimension C(h)C(h), recovered from the exponents by a Legendre transform; a broader or more asymmetric C(h)C(h) means stronger intermittency. The phenomenon has been recognized since Batchelor and Townsend's 1949 hot-wire measurements, and Kolmogorov's refined similarity hypothesis (1962) tied intermittent velocity statistics to the intermittency of local dissipation.

The von Kármán flow — fluid stirred between two counter-rotating impellers in a closed cylinder — is a canonical closed turbulent flow. It is globally inhomogeneous and anisotropic, with a turbulent shear layer (a cylindrical mixing layer separating the two impeller-driven recirculation cells) and a stagnation point at mid-height. It is one of few configurations where matched high-Reynolds-number experiments (stereoscopic and tomographic particle image velocimetry, SPIV and TPIV, measuring planar or volumetric velocity fields) and high-resolution direct numerical simulation (DNS; here a spectral/finite-element computation with about 3×1083\times10^8 grid points — 250 azimuthal Fourier modes plus finite elements in the meridional plane, equivalent grid 400×800×509400\times800\times509 — at Taylor-scale Reynolds number Rλ≈72R_\lambda\approx72, the standard turbulence-strength measure built on the root-mean-square velocity fluctuation and the Taylor microscale, with 21 statistically uncorrelated snapshots) can be realized in the same geometry.

A key modern tool in this program is the local interscale energy transfer DℓD_\ell: following Duchon and Robert's (2000) weak-solution energy balance and Dubrulle's (2019) construction, spatial filtering of the incompressible Navier–Stokes energy budget yields, at each point and scale ℓ\ell, the energy flux from scales larger than ℓ\ell to smaller ones, generalizing the Kármán–Howarth relation to non-homogeneous flows. Earlier measurements in the same facility had characterized extreme events of this 'inertial dissipation' (Saw et al. 2016). Faller et al. (2021) computed wavelet structure functions of the velocity (SWS_W), of the solenoidal (vortical) part of the flow (SΩS_\Omega), and of the local transfer (SDS_D), their multifractal spectra, and joint statistics of transfer and vorticity ω=∇×u\omega=\nabla\times u. Their findings: (a) velocity, vortical and transfer structure functions all obey a generalized extended scaling (extended self-similarity: power-law scaling of SpS_p against S3S_3 rather than against ℓ\ell itself, which extends the observable scaling range), and the velocity and vorticity spectra nearly coincide, supporting a local refined similarity hypothesis; (b) the transfer spectrum CDC_D is milder — more peaked around its most probable exponent — than the velocity spectrum CWC_W; (c) in joint probability densities, extreme energy transfers occur at only moderate vorticity while extreme vorticity is essentially independent of transfer, so the maxima of the two fields are spatially displaced (as previously observed in the same experiment); (d) the DNS joint density displays a highly correlated linear tail associated with shear-layer vortices, at a location reminiscent of where Luo and Hou (2014) computed a potentially self-similar blowing-up solution of the (inviscid) axisymmetric Euler equations in a comparable geometry; (e) conditioned on the sign of the transfer, upscale (negative) transfers are less intermittent than downscale ones; and (f) the transfer statistics obey a log-universality, collapsing across Reynolds numbers when rescaled by log⁡Rλ\log R_\lambda, generalizing earlier results of Geneste et al. (2019).

These findings sit inside a live debate on the mechanism of the turbulent cascade: whether intense small-scale dynamics are organized around vortex tubes (intense vorticity stretched by ambient strain) or around strain sheets, and whether the cascade is driven by vortex stretching (intensification of vorticity by the strain field through which it is advected) or by strain self-amplification (nonlinear self-intensification of the strain field; Johnson 2020; Buaria and Pumir 2026). What the correlation measurements cannot reveal is the direction of the interaction, the dynamical nature of the extreme objects, and whether the picture survives outside this particular flow — the gaps the source paper itself identified.

Problem Statement

Determine the dynamical mechanism — and its universality — underlying the observed intermittency of the local energy cascade in the turbulent von Kármán flow, by resolving the four coupled issues left open by Faller et al. (2021):

  1. Causal direction (the core). Establish whether local interscale energy transfer drives the intensification of vorticity, or whether intense vortical structures generate the extreme transfers — that is, settle, from time-resolved three-dimensional data (lagged conditional statistics or controlled perturbations), the dynamical relation between the two fields whose maxima are observed to be spatially displaced.

  2. Nature of the extreme structures. Establish whether the shear-layer vortices that produce the highly correlated tail of the transfer–vorticity joint statistics are self-similar quasi-singular structures — in the sense of approaching Euler-equation blow-up dynamics of the Luo–Hou type — that dominate the scaling of large-order structure functions, or whether they are ordinary intense vortices, and what their lifecycle in space and time is.

  3. Origin of the milder transfer intermittency. Decide whether the multifractal spectrum of the local energy transfer is milder than that of the velocity because finite spatial resolution misses the largest transfer events, or because of a genuine physical difference between the intermittency of vorticity and of interscale transfer at the smallest scales.

  4. Universality. Determine whether the transfer–vorticity correlations, the dominance (or not) of quasi-singular structures, and the log-universality of the transfer statistics extend to turbulent flows lacking the von Kármán shear layer and stagnation point, or are specific to this geometry.

The components are linked: 1 and 2 are the dynamical and structural faces of the same mechanism; 3 tests whether the measured transfer statistics can be taken at face value when building that mechanism; 4 tests whether the mechanism is a universal feature of turbulence. A resolution identifies the mechanism and states, with evidence, the answer to each of the four components; progress on 2–4 alone, without settling the causal question, does not complete the problem.

References

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