Active and adaptive optics for the Carlina Hypertelescope Technology roadmap for future interferometric facilities, Proceedings of the European Interferometry Initiative Workshop organized in the context of the 2005 Join European and National Astronomy Meeting "Distant Worlds", 6 - 8 July 2005, Liège University, Institute of Astrophysics, Edited by J. Surdej, D. Caro, and A. Detal

H. Le Coroller; V. Borkowski; J. Dejonghe; A. Labeyrie

Bulletin de la Société Royale des Sciences de Liège

0037-9565 1783-5720

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H. Le Coroller, V. Borkowski, J. Dejonghe & A. Labeyrie

Active and adaptive optics for the Carlina Hypertelescope
Technology roadmap for future interferometric facilities, Proceedings of the European Interferometry Initiative Workshop organized in the context of the 2005 Join European and National Astronomy Meeting "Distant Worlds", 6 - 8 July 2005, Liège University, Institute of Astrophysics, Edited by J. Surdej, D. Caro, and A. Detal

(Volume 74 - Année 2005 — Numéros 1-2- 3)

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Abstract

We describe a wave sensing method developed for the diluted aperture of the Carlina hypertelescope and other instruments having non-monolithic mirrors. Carlina is configured like a diluted version of the Arecibo radio-telescope. The diluted primary mirror is made of fixed co-spherical segments widely spaced with respect to their size. Above this diluted mirror a helium balloon carries a gondola containing the focal optics and detector. Following the first fringes obtained on Vega with a prototype, we develop active and adaptive optics expected to respectively coherence and phase several tens of mirrors.

Om dit artikel te citeren:

H. Le Coroller, V. Borkowski, J. Dejonghe & A. Labeyrie, «Active and adaptive optics for the Carlina Hypertelescope», Bulletin de la Société Royale des Sciences de Liège [En ligne], Numéros 1-2- 3, Volume 74 - Année 2005, 139 - 145 URL : http://popups.ulg.be/0037-9565/index.php?id=3732.