For the past twenty years, fractal grids have shown their efficiency at generating long-lasting broadband turbulence. Reference studies have so far focused on developing the most canonical self-similar turbulence far downstream of the grid; the production region was stretched out, and the maximum turbulence intensities at the peak remained limited. We explore a new region of the parameter space of fractal square grids to accelerate turbulence production, shorten the wake-interaction length, and enhance the kinetic energy in the early stages of the decay. The length-to-thickness ratio (L_0/t_0) of the first iteration is much lower than in typical grids reported in the literature, yielding peak turbulence intensities of 21–27% within (x/L_0 < 3). The experiments were conducted in a recirculating hydro-channel facility using Particle Image Velocimetry for spatially extended data and Laser Doppler Velocimetry for time-resolved centerline statistics. A sweep of progressively smaller PIV fields of view, with vector spacing down to (Delta x / eta approx 1.3), is used in the decay region to approach the dissipative range. The analysis focuses on the production region and the early-decay region within the wake-interaction length ((x < x_*)) and combines centerline statistics, characteristic length scales and the spectral signature along the flow. A scale-by-scale spectral assessment, benchmarked against forced-isotropic DNS, shows that local isotropy is recovered over the reliable resolved wavenumber range, whereas global derivative-based indicators (K_1) and (K_3) remain affected by large-scale anisotropy and finite PIV resolution. The results are consistent with the non-equilibrium scaling reported in earlier studies of fractal-grid-generated turbulence. The new grids, however, reveal that the dissipation scaling (C_epsilon sim sqrt{text {Re}_{L_0}}/text {Re}_lambda ) no longer holds when the geometry is extended to low (L_0/t_0) ratios. Using (text {Re}_{t_0}) based on the largest-bar thickness restores the collapse with the literature, indicating that the relevant global Reynolds number is set by the vortex-shedding scale at which energy is initially injected, rather than by the largest geometric scale of the grid.


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