Share Email Print
cover

Proceedings Paper

Analysis of inner geometric noise influence on image quality of large aperture segmented adaptive telescopes
Author(s): Yurij Petrovich Shumilov; Peter Alexseevich Bakut; Olga M. Ershova
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

Distortions, induced by angular and longitudinal errors of telescope segments aligning, are analyzed. Two mechanisms of images averaging are modeled and analytically investigated. Temperature and other slow fluctuations of telescope mirror segments geometric parameters cause one of them. Correlation time of that process is of the order of several hours. That mechanism is investigated in reference 1. Correlation time of the other process is determined by receiving device material time constant. In the second case the certain amount of mirror segments is necessary for the averaging. If the first case, in principle, compensation is possible, the distortions can't be compensated in the second one. It leads to existing in the image some constant component, called 'inner geometric noise' (IGN). We obtained illustrating dependencies and evaluation of the IGN influence on telescope vision range.

Paper Details

Date Published: 29 January 2002
PDF: 6 pages
Proc. SPIE 4538, Optics in Atmospheric Propagation and Adaptive Systems IV, (29 January 2002); doi: 10.1117/12.454402
Show Author Affiliations
Yurij Petrovich Shumilov, Institute of Problem of Informational Resources (Russia)
Peter Alexseevich Bakut, Institute of Problem of Informational Resources (Russia)
Olga M. Ershova, Institute of Problem of Informational Resources (Russia)


Published in SPIE Proceedings Vol. 4538:
Optics in Atmospheric Propagation and Adaptive Systems IV
Anton Kohnle; John D. Gonglewski; Thomas J. Schmugge, Editor(s)

© SPIE. Terms of Use
Back to Top