Paper
12 October 2004 A pupil plane technique for sensing and correcting large phase aberrations
Author Affiliations +
Abstract
Large deployable space telescopes like the James Webb Space Telescope (JWST) may have large errors after deployment that must be corrected in situ. One approach is to correct the errors successively. In this paper, we present a new approach to correct large phase aberrations during the coarse figuring stage of the initial alignment. Intensity data is obtained from multiple planes: pupil plane and additional planes in the nearfield of the pupil plane. The irradiance transport equation is used in a new manner used to estimate the phase aberrations at the pupil. The technique was demonstrated in the lab to estimate phase aberrations approaching 20 waves.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gopal Vasudevan and Robert D. Reardon "A pupil plane technique for sensing and correcting large phase aberrations", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.551977
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Actuators

Mirrors

Collimation

James Webb Space Telescope

Space telescopes

Near field

Cameras

RELATED CONTENT

Non-redundant masking ideas on JWST
Proceedings of SPIE (August 28 2014)
JWST mirror and actuator performance at cryo-vacuum
Proceedings of SPIE (July 06 2018)
HYPATIA and STOIC an active optics system for a...
Proceedings of SPIE (July 29 2016)
The Magellan Telescopes: a performance update
Proceedings of SPIE (August 04 2010)

Back to Top