Share Email Print

Proceedings Paper

High-resolution astronomical observations using deconvolution from wavefront sensing
Author(s): Vincent Michau; T. Marais; Jean Laurent; Jerome Primot; Jean-Claude Fontanella; Michel Tallon; Jesus Jimenez Fuensalida
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

Deconvolution from wavefront sensing is a new technique of high-resolution imaging through atmospheric turbulence developed at ONERA. The capabilities of the method have been demonstrated during first laboratory experiments. A deconvolution experimental set-up was installed on the 4.2 m William Herschel telescope on La Palma in November 1990. The results obtained during these observations are presented: the astronomical sources were observed at optical wavelengths; the resolution improvement reached a factor greater than 10.

Paper Details

Date Published: 1 July 1991
PDF: 8 pages
Proc. SPIE 1487, Propagation Engineering: Fourth in a Series, (1 July 1991); doi: 10.1117/12.46580
Show Author Affiliations
Vincent Michau, ONERA (France)
T. Marais, ONERA (France)
Jean Laurent, ONERA (France)
Jerome Primot, ONERA (France)
Jean-Claude Fontanella, ONERA (France)
Michel Tallon, Imperial College of Science, Technology and Medicine (United Kingdom)
Jesus Jimenez Fuensalida, Instituto de Astrofisica de Canarias (Spain)

Published in SPIE Proceedings Vol. 1487:
Propagation Engineering: Fourth in a Series
Luc R. Bissonnette; Walter B. Miller, Editor(s)

© SPIE. Terms of Use
Back to Top