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Last name: LANTERI
First name: H.
MNRAS, 368, pp. 1456-1462 (2006)
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Atmospheric turbulence is responsible of the spatio-temporal fluctuations in astronomical object images obtained by means of ground-based telescopes. They are due to wave-front degradations present at the entrance of the instrument pupil plane. We first establish in this paper the formulation of the angle-of-arrival angular structure function...
Atmospheric turbulence is responsible of spatio-temporal fluctuations of astronomical object images obtained by means of ground-based telescopes. The image motion is due to the angle formed by the pupil plane with the wave-front slope all over the pupil. This defines an averaged angle of arrival which may be also considered at each point of the...
J. Comp. Appl. Math., 198, pp. 321-331 (2006)
Astron. & Astrophys., 409, pp. 387-394 (2003)
iAO/COSI/IP/SRS OSA Meeting, OSA/SRS n/a, (2006)
International audience
International audience
In previous papers we proposed methods and software for the restoration of images provided by Fizeau interferometers such as LINC-NIRVANA (LN), the German-Italian beam combiner for the Large Binocular Telescope (LBT). It will provide multiple images of the same target corresponding to different orientations of the baseline. Therefore LN will...
J. Comp. Appl. Math., 198, p. 321 (2007)
Astron. & Astrophys., 448, p. 1217 (2006)
International audience