We review the operating principles of noncollinear acousto-optic tunab
le filters (AOTF's), emphasizing the use of two orthogonally polarized
beams for narrow-band imaging. Spectral characterization and spectral
broadening measurements of commercially available AOTF's agree with t
heoretical predictions and reveal difficulties associated with imaging
noncollimated light. An AOTF imaging spectropolarimeter for ground-ba
sed astronomy that uses CCD's has been constructed at NASA Goddard Spa
ce Flight Center. It uses a TeO2 noncollinear AOTF and a simple optica
l relay assembly to produce side-by-side orthogonally polarized spectr
al images. We summarize the instrument design and initial performance
tests. We include sample spectral images acquired at the Goddard Geoph
ysical and Astronomical Observatory.