  We investigate clusters of misaligned (inclined) tori orbiting a central
static Schwarzschild black hole. To this purpose we considered a set of
geometrically thick, pressure supported, perfect fluid tori analyzing purely
hydrodynamic models. We study the tori collision emergence and, consequently,
the stability properties of the aggregates composed by tori with different
inclination angles relative to a fixed distant observer. The aggregate of
tilted tori is modeled as a single orbiting configuration, by introducing a
leading function governing the distribution of toroids around the black hole
attractor. Eventually the tori agglomerate can be seen, depending on the tori
thickness, as a (multipole) gobules of orbiting matter, with different toroidal
spin orientations , covering the embedded central black hole. These systems are
shown to include tori with emerging instability phase related to accretion onto
the central black hole. Therefore we provide an evaluation of quantities
related to tori energetics such as the mass-flux, the enthalpy-flux, and the
flux thickness depending on the model parameters for polytropic fluids.
Consequently this analysis places constraints on the existence and properties
of tilted tori and aggregate of misaligned disks. Some notes are included on
aggregates including proto-jets, represented by open cusped solutions
associated to the geometrically thick tori.
