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Proceedings Paper

High Resolution Interferometric Imaging Using A Large Optical Telescope
Author(s): R. H. Frater; J. G. Robertson; J. D. O'Sullivan
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Paper Abstract

Large optical telescopes (diameter 'Am) used for astronomy have a theoretical diffraction-limited angular resolution of ~0.03 arcsec. However, when used for conventional long-exposure imaging, the resolution is degraded to ~l arcsec by phase perturbations due to the Earth's atmosphere. We discuss methods to overcome this so-called "seeing" limit, with particular reference to a method based on the use of a mask in the aperture plane of the telescope. We discuss results from preliminary tests of this method.

Paper Details

Date Published: 18 May 1987
PDF: 4 pages
Proc. SPIE 0702, International Topical Meeting on Image Detection and Quality, (18 May 1987); doi: 10.1117/12.966771
Show Author Affiliations
R. H. Frater, CSIRO Division of Radiophysics (Australia)
J. G. Robertson, Anglo-Australian Observatory (Australia)
J. D. O'Sullivan, CSIRO Division of Radiophysics (Australia)

Published in SPIE Proceedings Vol. 0702:
International Topical Meeting on Image Detection and Quality
Lucien F. Guyot, Editor(s)

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