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We present the first to date three-dimensional high-resolution hydrodynamicalsimulation tracing the non-equilibrium ionization evolution (using the EboraeAtomic and Molecular Plasma Emission Code - E(A+M)PEC) of the Local Bubble andLoop I superbubbles embedded in a turbulent supernova-driven interstellarmedium.

A Non-Equilibrium Ionization Model of the Local and Loop I Bubbles - Tracing the Ovi Distribution