Adaptive optics (AO) combines technologies that enable the correction of th
e wavefront distortion caused by the earth's atmospheric turbulence in real
time. Adaptive secondary mirror (ASM) systems have been proposed and are n
ow being developed. ASMs have advantages over conventional AO systems in te
rms of throughput, polarization and IR emissivity. Previously, we reported
the design of an ASM demonstrator along with its predicted performance. We
now report the construction techniques and the results from the preliminary
static and dynamic testing of such a demonstrator. In particular, assembly
methods that preserve the optical quality of the mirror are presented alon
g with experimentally measured mirror influence functions and closed loop t
ip/tilt performance. (C) 2000 society of Photo-Optical Instrumentation Engi
neers.