  Radiative flavor models where the hierarchies of Standard Model (SM) fermion
masses and mixings are explained via loop corrections are elegant ways to solve
the SM flavor puzzle. Here we build such a model in the context of Mini-Split
Supersymmetry (SUSY) where both flavor and SUSY breaking occur at a scale of
1000 TeV. This model is consistent with the observed Higgs mass, unification,
and WIMP dark matter. The high scale allows large flavor mixing among the
sfermions, which provides part of the mechanism for radiative flavor
generation. In the deep UV, all flavors are treated democratically, but at the
SUSY breaking scale, the third, second, and first generation Yukawa couplings
are generated at tree level, one loop, and two loops, respectively. Save for
one, all the dimensionless parameters in the theory are O(1), with the
exception being a modest and technically natural tuning that explains both the
smallness of the bottom Yukawa coupling and the largeness of the Cabibbo angle.
