Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-25T22:12:03.446Z Has data issue: false hasContentIssue false
  • English
  • Français

Restoration Over Fields of View Wider than the Isoplanatic Patch

Published online by Cambridge University Press:  19 July 2016

G. Thorpe  and
D. Fraser
G. Thorpe
Affiliation:
Department of Electrical Engineering, University of New South Wales, ADFA
D. Fraser
Affiliation:
Department of Electrical Engineering, University of New South Wales, ADFA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This paper presents the results of a preliminary investigation into the problems in through-the-atmosphere image restoration which are more suited to data from a small telescope, i.e., one having a diameter of about 0.5 m, using techniques of image geometric transformation (and eventually, parallel image processing) in their solution. We have imaged bright objects, over fields of view which subtend angles greater than those in most “large” telescope experiments, i.e., between 40 and 100 arc sec, for example, where the isoplanatic assumptions are less valid.

Type
Imaging Theory
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 221 - 223
Copyright
Copyright © Kluwer 1994 

References

[1] Stewart McKechnie, T., “Light propagation through the atmosphere and the properties of images formed by large ground-based telescopes”, J. Opt. Soc. Am. A/vol. 8, No. 2 Febuary 1991.Google Scholar
[2] Irani, Michal and Peleg, Shmuel, “Improving Resolution by Image Registration”, CVGIP Graphical Models and Image Processing vol 53, No. 3, May, pp 231–239, 1991.CrossRefGoogle Scholar