  I present here a review of Large-Scale Structure (LSS) studies using clusters
of galaxies. First, I re-evaluate the `pros' and `cons' of using clusters for
such studies, especially in this era of large galaxy redshift surveys.
Secondly, I provide an historical review of the Cluster Correlation Function
and show that the latest measurements of xi_cc from Abell and X-ray catalogs
are in excellent agreement. Thirdly, I review the latest measurements of the
power spectrum of clusters which provide strong constraints on the cosmological
parameters e.g. Omega_m and models of structure formation. Moreover, I
highlight the recent discovery of ``Baryon Wiggles'' in the local cluster p(k)
which is in perfect agreement with the recent CMB data. Lastly, I examine
recent advances in the measurement of the X-ray Cluster Luminosity Function and
emphasize the importance of accurately determining the selection function of
future cluster surveys.
