High-resolution astronomical observations using deconvolution from wavefront sensing

Details High-resolution astronomical observations using deconvolution from wavefront sensing High-resolution astronomical observations using deconvolution from wavefront sensing

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1487...64m&link_type=abstract

Proc. SPIE Vol. 1487, p. 64-71, Propagation Engineering: Fourth in a Series, Luc R. Bissonnette; Walter B. Miller; Eds.

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

High-resolution astronomical observations using deconvolution from wavefront sensing does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High-resolution astronomical observations using deconvolution from wavefront sensing, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-resolution astronomical observations using deconvolution from wavefront sensing will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-864349