  Kinetic simulations of relativistic turbulence have significantly advanced
our understanding of turbulent particle acceleration. Recent progress has
highlighted the need for an updated acceleration theory that can account for
acceleration within the plasma's coherent structures. Here, we investigate how
turbulent intermittency models connect statistical fluctuations in turbulence
to regions of high dissipation. This connection is established by employing a
generalized She-Leveque model to describe the exponents $\zeta_p$ for the
structure functions $S^p \propto l^{\zeta_p}$. The fitting of the scaling
exponents provide us with a measure of the co-dimension of the dissipative
structures, and we subsequently measure their filling fraction. We perform our
analysis for a range of magnetizations $\sigma$ and magnetic field fluctuations
${\delta B_0}/{B_0}$. We find that increasing the values of $\sigma$ and
${\delta B_0}/{B_0}$ allows the cascade to break sheets into smaller regions of
dissipation that resemble chains of plasmoids. However, as their dissipation
increases, the dissipative regions become less volume filling. With this work
we aim to inform future turbulent acceleration theories that incorporate
particle energization from interactions with coherent structures within
relativistic turbulence.
