Jet collision with accreting tori around SMBHs GRHD and light surface constraints in aggregates of misaligned tori

We explore the possibility of jet collisions with accreting tori orbiting around SMBHs. The analysis provides constraints on formation and observational evidences host configurations. use a GRHD model, investigating light surfaces contraints in aggregates misaligned central static Schwarzschild black hole. Each (toroidal) configuration agglomeration is geometrically thick, pressure supported, perfect fluid torus. Aggregates include proto-jets, open cusped solutions associated to thick tori. Collision emergence stability properties are considered at different inclination angles relative fixed distant observer. relate relevant frequencies configurations specific angular momentum, separating related fluids hydrodynamics geometric backgrounds. analyze existence supporting jet-emission. discuss orbit-replicas that could shadowing effects replicas emissions two regions, close far from BH (horizon shells). investigation clarifies role gradients matter essential radial gradient determination disk verticality. Finally we toroidal magnetic field be collimation proto-jets.