Paper
26 April 1995 PAMELA: phase I testing and verification on a 0.5-m diameter telescope with a 36-segment adaptive primary mirror
Gregory H. Ames, Richard T. Howard, Jeffrey L. Lindner, Edward E. Montgomery IV, Alan F. Patterson, John M. Rakoczy, Glenn W. Zeiders Jr., Henry B. Waites
Author Affiliations +
Abstract
The Phased Array Mirror, Extendible Large Aperture (PAMELA) prototype telescope phase I testing and verification has been completed. The prototype telescope is the first to have a fully adaptive primary mirror which consists of 36 hexagonal injection-molded Pyrex segments that are seven centimeters flat-to-flat. The segments are mounted on three long-throw voice-coil actuators for tip, tilt, and piston motion. The segments' tilts are measured with a Hartmann- Shack wavefront sensor, and the piston errors between adjacent segments are measured via inductive edge-sensors. The 0.5 meter telescope was successfully operated with simultaneously closed tilt and piston control loops for the entire array. Phase I test and verification results are shown for the closed loop operations.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gregory H. Ames, Richard T. Howard, Jeffrey L. Lindner, Edward E. Montgomery IV, Alan F. Patterson, John M. Rakoczy, Glenn W. Zeiders Jr., and Henry B. Waites "PAMELA: phase I testing and verification on a 0.5-m diameter telescope with a 36-segment adaptive primary mirror", Proc. SPIE 2376, Laser Power Beaming II, (26 April 1995); https://doi.org/10.1117/12.208202
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Mirrors

Telescopes

Actuators

Calibration

Control systems

Phased arrays

RELATED CONTENT


Back to Top