  We present James Webb Space Telescope MIRI data of the inner ~3x2 kpc^2 of
the galaxy IC5063, in which the jets of a supermassive black hole interact with
the gaseous disk they are crossing. Jet-driven outflows were known to be
initiated along or near the jet path, and the stability conditions of clouds
were known to vary because of these outflows. The MIRI data, of unprecedented
resolution and sensitivity in the infrared, now reveal that there are more than
ten discrete regions with outflows, nearly doubling the number of such known
regions. Outflows exist near the radio lobes, at the nucleus, in a biconical
structure perpendicular to the jet, and in a bubble moving against the disk. In
some of them, velocities above escape velocity are observed. Stratification is
also observed, with higher ionization or excitation gas attaining higher
velocities. More outflows and bow shocks, found further away from the nucleus
than the radio lobes, in regions without significant radio emission, reveal the
existence of past or weak radio jets that interacted with the interstellar
medium. The coincidence of the bow shocks with the optical extended emission
line region (EELR) suggests that the jets also contributed to the gas
ionization. Maps of the H2 gas excitation temperature, T_ex, indicate that the
molecular gas is most excited in regions with radio emission. There, T_ex is
more than 100K higher than in the EELR interior. We argue that a combination of
jet-related shocks and cosmic rays is likely responsible for this excess
molecular gas excitation.
