  We present the second data release (DR2) of the Far-Infrared Polarimetric
Large-Area CMZ Exploration (FIREPLACE) survey. This survey utilized the
Stratospheric Observatory for Infrared Astronomy (SOFIA) High-resolution
Airborne Wideband Camera plus (HAWC+) instrument at 214 $\mu$m (E-band) to
observe dust polarization throughout the Central Molecular Zone (CMZ) of the
Milky Way. DR2 consists of observations that were obtained in 2022 covering the
region of the CMZ extending roughly from the Brick to the Sgr C molecular
clouds (corresponding to a roughly 1$^{\circ}$ $\times$ 0.75$^{\circ}$ region
of the sky). We combine DR2 with the first FIREPLACE data release to obtain
full coverage of the CMZ (a 1.5$^{\circ}$ $\times$0.75$^{\circ}$ region of the
sky). After applying total and polarized intensity significance cuts on the
full FIREPLACE data set we obtain $\rm\sim$65,000 Nyquist-sampled polarization
pseudovectors. The distribution of polarization pseudovectors confirms a
bimodal distribution in the CMZ magnetic field orientations, recovering field
components that are oriented predominantly parallel or perpendicular to the
Galactic plane. These magnetic field orientations indicate possible connections
between the previously observed parallel and perpendicular distributions. We
also inspect the magnetic fields toward a set of prominent CMZ molecular clouds
(the Brick, Three Little Pigs, 50 km s$\rm^{-1}$, Circum-nuclear Disk, CO
0.02-0.02, 20 km s$\rm^{-1}$, and Sgr C), revealing spatially varying magnetic
fields that generally trace the morphologies of the clouds. We find evidence
that compression from stellar winds and shear from tidal forces are prominent
mechanisms influencing the structure of the magnetic fields observed within the
clouds.
