Physics – Optics
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1168..201g&link_type=abstract
IN: Current developments in optical engineering and commercial optics; Proceedings of the Meeting, San Diego, CA, Aug. 7-11, 198
Physics
Optics
Aberration, Faint Object Camera, Hubble Space Telescope, Misalignment, Optical Correction Procedure, Point Spread Functions, Optical Properties, Pixels, Pupil Size, Spaceborne Telescopes
Scientific paper
A backup scheme for correcting misalignment-dependent aberrations of the HST is described which uses a phase retrieval algorithm to compute secondary mirror misalignments from measured point spread function (PSF) data at two different field locations. The PSF data are obtained from the Faint Object Camera and the Wide Field Planetary Camera. Comparison pupil functions are written in terms of annular Zernike Polynomial. At the two field locations of the instruments, artificial PSFs are generated from FFTs of the respective pupil functions, and the mean square differences between the actual PSFs and constructed PSFs are mimimized with respect to the Zernike Polynomial coefficients. Thus, two sets of coefficients are obtained, one for each of the field positions. Statistical regression analysis is then used to determine the misalignments as a function of the aberration coefficients.
Grey Louis D.
Lyon Richard G.
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