We describe the HEMT Advanced Cosmic Microwave Explorer (HACME), a balloon-
borne experiment designed to measure subdegree-scale cosmic microwave backg
round anisotropy over hundreds of deg(2), using a unique two-dimensional sc
anning strategy. A spinning flat mirror that is canted relative to its spin
axis modulates the direction of beam response in a nearly elliptical path
on the sky. The experiment was successfully flown in 1996 February, achievi
ng near laboratory performance for several hours at float altitude. A map f
ree of instrumental systematic effects is produced for a 3.5 hr observation
of 630 deg(2), resulting in a flat-band power upper limit of [l(l + 1)C-I/
(2 pi)](0.5) < 77 mu K at l = 38(-20)(+25) (95% confidence). The experiment
design, flight operations, and data, including atmospheric effects and noi
se performance, are discussed.