  We present results of a joint {\sl Chandra} and {\sl XMM-Newton} analysis of
the Fornax Cluster, the nearest galaxy cluster in the southern sky. Signatures
of merger-induced gas sloshing can be seen in the X-ray image. We identify four
sloshing cold fronts in the intracluster medium, residing at radii of 3\,kpc
(west), 10\,kpc (northeast), 30\,kpc (southwest) and 200\,kpc (east). Despite
spanning over two orders of magnitude in radius, all four cold fronts fall onto
the same spiral pattern that wraps around the BCG NGC~1399, likely all
initiated by the infall of NGC~1404. The most evident front is to the
northeast, 10\,kpc from the cluster center, which separates low-entropy
high-metallicity gas and high-entropy low-metallicity gas. The metallicity map
suggests that gas sloshing, rather than an AGN outburst, is the driving force
behind the redistribution of the enriched gas in this cluster. The innermost
cold front resides within the radius of the strong cool core. The sloshing time
scale within the cooling radius, calculated from the Brunt-V$\ddot{\rm
a}$s$\ddot{\rm a}$l$\ddot{\rm a}$ frequency, is an order of magnitude shorter
than the cooling time. It is plausible that gas sloshing can contribute to the
heating of the cool core, provided that gas of different entropies can be mixed
effectively via Kelvin-Helmholtz instability. The estimated age of the
outermost front suggests that this is not the first infall of NGC~1404.
