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We consider agglomerates of misaligned, pressure supported tori orbiting aSchwarzschild black hole. A leading function is introduced, regulating thetoroids distribution around the central static attractor-it enables to modelthe misaligned tori aggregate as a single orbiting (macro--)configuration. Wefirst analyze the leading function for purely hydrodynamical perfect fluidtoroids. Later, the function is modified for presence of a toroidal magneticfield. We study the constraints on the tori collision emergence and theinstability of the agglomerates of misaligned tori with general relativeinclination angles. We discuss the possibility that the twin peakhigh-frequency quasi-periodic oscillations (HF-QPOs) could be related to theagglomerate inner ringed structure. The discrete geometry of the system isrelated to HF-QPOs considering several oscillation geodesic models associatedto the toroids inner edges. We also study possible effect of the torigeometrical thickness on the oscillatory phenomena.

Limiting effects in clusters of misaligned toroids orbiting static SMBHs