Share Email Print

Proceedings Paper

Compensation with models for the optics design for a large FOV star sensor
Author(s): Hua Xie; Junfeng F. Xu; Huaifeng F. Li; Caihong H. Sun; Shengzheng Z. Jin; Guoxiang X. Ai
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

This paper depicts the general analysis before designing optics for an APS based star sensor. The high accuracy requirement and low sensitivity of APS make the optics overcritical. To avoid the extreme difficulty in optics, we abstract the PSF models in sub-pixel scale as the compensation for the distortion error. Both centroid and correlation algorithm are used to determine the spot center. The result of the simulation is presented in the text.

Paper Details

Date Published: 16 September 2004
PDF: 8 pages
Proc. SPIE 5497, Modeling and Systems Engineering for Astronomy, (16 September 2004); doi: 10.1117/12.563326
Show Author Affiliations
Hua Xie, Peking Univ. (China)
National Astronomical Observatories (China)
Technical Univ. Brunswick (Germany)
Junfeng F. Xu, National Astronomical Observatories (China)
Huaifeng F. Li, National Astronomical Observatories (China)
Caihong H. Sun, National Astronomical Observatories (China)
Shengzheng Z. Jin, National Astronomical Observatories (China)
Guoxiang X. Ai, National Astronomical Observatories (China)

Published in SPIE Proceedings Vol. 5497:
Modeling and Systems Engineering for Astronomy
Simon C. Craig; Martin J. Cullum, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?