Image-Stabilization Systems - Introduction to Image Stabilization - page 83

Image-Stabilization Systems 83

Figure 7.9 Tilt mirrors presently in use at NPOI.

References
1.

White, N.M., D. Mozurkewich, J.T. Armstrong, D.J. Hutter, K.J. Johnston, J.
Clark, L. Ha, “Infrastructure and the layout of the Navy Prototype Optical In-
terferometer at the Lowell Observatory,” Proceedings of SPIE , 3350 , 471-477
(1998).

2. Benson, J.A., D. Mozurkewich, S.M. Jefferies, “Active optical fringe tracking

at NPOI,” Proceedings of SPIE , 3350 , 493-496 (1998).

Paul Wild Observatory
The long-baseline Sydney University Stellar Interferometer (SUSI), with a 640-m
maximum baseline, is located at the Paul Wild Observatory in New South Wales,
Australia. Beam stabilization is provided through an active tip-tilt system.

References
1.

Tango, W.J., “Status of the SUSI program,” Proceedings of SPIE , 4838 ,28-32
(2003).