Paper
13 September 2012 Fine optical alignment correction of astronomical spectrographs via in-situ full-field moment-based wavefront sensing
Author Affiliations +
Abstract
The image moment-based wavefront sensing (IWFS) utilizes moments of focus-modulated focal plane images to determine modal wavefront aberrations. This permits fast, easy, and accurate measurement of wavefront error (WFE) on any available finite-sized isolated targets across the entire focal plane (FP) of an imaging system, thereby allowing not only in-situ full-field image quality assessment, but also deterministic fine alignment correction of the imaging system. We present an experimental demonstration where fine alignment correction of a fast camera system in a fiber-fed astronomical spectrograph, called VIRUS, is accomplished by using IWFS.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hanshin Lee, Gary J. Hill, Sarah E. Tuttle, and Brian L. Vattiat "Fine optical alignment correction of astronomical spectrographs via in-situ full-field moment-based wavefront sensing", Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84500V (13 September 2012); https://doi.org/10.1117/12.926741
Lens.org Logo
CITATIONS
Cited by 11 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Spectrographs

Cameras

Modulation

Wavefronts

Point spread functions

Wavefront sensors

RELATED CONTENT


Back to Top