High resolution imaging at large telescopes

Details High resolution imaging at large telescopes High resolution imaging at large telescopes

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980oits.conf..401n&link_type=abstract

Optical and Infrared Telescopes for the 1990's. Proceedings of the conference held 7-12 January, 1980 in Tucson, AZ. Edited by

Statistics

Applications

High Resolution, Image Reconstruction, Imaging Techniques, Speckle Patterns, Telescopes, Bias, Digital Techniques, Fourier Transformation, Instrument Compensation, Signal To Noise Ratios, Video Data

Scientific paper

Image recovery at a resolution limited only by diffraction is now possible at large telescopes. The theory of speckle image reconstruction is explained and the current status of a video recording and digitization system for the reconstruction procedure is described. Potential applications of the process when used with very large telescopes are discussed. The constraints on telescope design imposed by these techniques are listed.

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