  We present observations of the stripped Virgo Cluster spiral NGC 4522, a
clear, nearby example of a galaxy currently undergoing ISM-ICM stripping.
Utilizing SparsePak integral field spectroscopy on the WIYN 3.5m telescope and
GALEX UV photometry, we present an analysis of the outer disk (r > 3 kpc)
stellar population of this galaxy, beyond the HI and Halpha truncation radius.
We find that the star formation in the gas-stripped outer disk ceased very
recently, ~100 Myr ago, in agreement with previous claims that this galaxy is
currently being stripped. At the time of this stripping, data and models
suggest that the galaxy experienced a modest starburst. The stripping is
occurring in a region of the cluster well outside the cluster core, likely
because this galaxy is experiencing extreme conditions from a dynamic ICM due
to an ongoing sub-cluster merger. The outer disk has a spectrum of a K+A
galaxy, traditionally observed in high-redshift cluster galaxies. In the case
of NGC 4522, a K+A spectrum is formed by simple stripping of the interstellar
gas by the hot intracluster medium. These data show K+A spectra can be created
by cluster processes and that these processes likely extend beyond the cluster
core.
