We describe recent work in the area of large, back-illuminated CCD ima
gers at M.I.T. Lincoln Laboratory as well as new technology applicable
to astronomy. We completed in 1995 the development of a 2560 x 1960-p
ixel frame-transfer imager that filled a 100-mm wafer and several back
-illuminated versions of this device were completed. More recently we
have begun the development, in collaboration with the U. of Hawaii, of
a three-side abuttable 2k x 4k CCD for a multi-chip focal plane. In t
he unused chord area of the wafer layout, we added test imagers as dev
elopment vehicles for blooming control and for the demonstration of a
CCD that is capable of charge transfer in all four directions. Ne expe
ct the latter to find application as an electronic means of performing
tip-tilt correction to compensate for atmospheric turbulence.