Ultra-lightweight telescope with MEMS adaptive optic for distortion correction.

Spahn, Olga Blum ; Cowan, William D. ; Shaw, Michael J. ; Adams, David Price ; Sweatt, William C. ; Dagel, Daryl James ; Grine, Alejandro J. ; Mani, Seethambal S. ; Resnick, Paul James ; Gass, Fawn Renee ; Grossetete, Grant David

Sandia National Laboratories

关键词: Remote Sensing;    Telescopes.;    Mirrors;    Microelectronics.;    Satellite Observation;   

DOI  :  10.2172/920763
RP-ID  :  SAND2004-6322
RP-ID  :  AC04-94AL85000
RP-ID  :  920763

美国|英语

来源: UNT Digital Library

【 摘 要 】

Recent world events have underscored the need for a satellite based persistent global surveillance capability. To be useful, the satellite must be able to continuously monitor objects the size of a person anywhere on the globe and do so at a low cost. One way to satisfy these requirements involves a constellation of satellites in low earth orbit capable of resolving a spot on the order of 20 cm. To reduce cost of deployment, such a system must be dramatically lighter than a traditional satellite surveillance system with a high spatial resolution. The key to meeting this requirement is a lightweight optics system with a deformable primary and secondary mirrors and an adaptive optic subsystem correction of wavefront distortion. This proposal is concerned with development of MEMS micromirrors for correction of aberrations in the primary mirror and improvement of image quality, thus reducing the optical requirements on the deployable mirrors. To meet this challenge, MEMS micromirrors must meet stringent criteria on their performance in terms of flatness, roughness and resolution of position. Using Sandia's SUMMIT foundry which provides the world's most sophisticated surface MEMS technology as well as novel designs optimized by finite element analysis will meet severe requirements on mirror travel range and accuracy.