  We discuss some recent integral field spectroscopy using the SAURON
instrument of a sample consisting of 24 early-type spirals, part of the SAURON
Survey, and 18 late-type spirals. Using 2-dimensional maps of their stellar
radial velocity, velocity dispersion, and absorption line strength, it is now
much easier to understand the nature of nearby galactic bulges. We discuss a
few highlights of this work, and point out some new ideas about the formation
of galactic bulges.
