Bibcode
Rodríguez, J. M.; Femenía, B.; Montilla, I.; Rodríguez-Ramos, L. F.; Marichal-Hernández, J. G.; Lüke, J. P.; López, R.; Díaz, J. J.; Martín, Y.
Bibliographical reference
1st AO4ELT conference - Adaptative Optics for Extremely Large Telescopes, held 22-26 June, 2009 in Paris, France. Edited by Y. Clénet, J.-M. Conan, Th. Fusco, and G. Rousset. EDP Sciences, 2010, id.05011
Advertised on:
2010
Citations
3
Refereed citations
3
Description
The CAFADIS camera is a new wavefront sensor (WFS) patented by the
Universidad de La Laguna. CAFADIS is a system based on the concept of
plenoptic camera originally proposed by Adelson and Wang [Single lens
stereo with a plenoptic camera, IEEE Transactions on Pattern Analysis
and Machine Intelligence 14 (1992)] and its most salient feature is its
ability to simultaneously measuring wavefront maps and distances to
objects [Wavefront and distance measurements using the CAFADIS camera,
in Astronomical telescopes, Marseille (2008)]. This makes of CAFADIS an
interesting alternative for LGS-based AO systems as it is capable of
measuring from an LGS-beacon the atmospheric turbulence wavefront and
simultaneously the distance to the LGS beacon thus removing the need of
a NGS defocus sensor to probe changes in distance to the LGS beacon due
to drifts of the mesospheric Na layer. In principle, the concept can
also be employed to recover 3D profiles of the Na Layer allowing for
optimizations of the measurement of the distance to the LGS-beacon.
Currently we are investigating the possibility of extending the
plenoptic WFS into a tomographic wavefront sensor. Simulations will be
shown of a plenoptic WFS when operated within an LGS-based AO system for
the recovery of wavefront maps at different heights. The preliminary
results presented here show the tomographic ability of CAFADIS.