| タイトル | Measuring Low-Order Aberrations in a Segmented Telescope |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110014871 |
| 著者（英） | Burns, Laura; Dumont, Philip; Ohara, Catherine; Green, Joseph; Redding, David; Petrone, Peter; Shi, Fang; Lowman, Andrew; Basinger, Scott |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2005-04-01 |
| 言語 | eng |
| 内容記述 | The in-focus PSF optimizer (IPO) is an algorithm for use in monitoring and controlling the alignment of the segments of a segmented-mirror astronomical telescope. IPO is so named because it computes wave-front aberrations of the telescope from digitized pointspread functions (PSFs) measured in infocus images. Inasmuch as distant astronomical objects that behave optically as point sources can typically be seen in almost any astronomical image, the main benefit afforded by IPO may be to enable maintenance of mirror-segment alignments without detracting from valuable scientific-observation time. IPO evolved from prescription-retrieval type algorithms. Prescription retrieval uses in-focus and out-of-focus PSFs to infer the state of an imaging optical system. The state, in this context, refers to the positions, orientations, and low-order figure errors of the optical elements in the system. Both prescription- retrieval and IPO use an iterative, nonlinear, least-squares optimizer to compute the optimal state parameters such that a digital computer-generated model image matches the digitized image acquired from the real system. The difference between IPO and prescription- retrieval algorithms is that IPO is specifically designed to utilize infocus images only. Although the restriction to in-focus images limits IPO to calculating only the lowest-order wave front aberrations, it also causes the resulting computation to take much less time because fewer degrees of freedom are included in the optimization process. In the prescription retrieval software developed at JPL, the model images are generated using the ray-trace/physical optics program, MACOS. IPO, on the other hand, uses a linear sensitivity matrix to compute the exit-pupil wave front from the system parameters; the wave front is then converted into a complex pupil field, which is then propagated to the image plane via a fast Fourier transform. This approach is computationally faster and requires less computer memory than is needed for prescription retrieval. |
| NASA分類 | Man/System Technology and Life Support |
| レポートNO | NPO-30733 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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