Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 308704.0, MPI für Astronomie / Publikationen_mpia
Eliminating perspective elongation for LGS based AO-systems at ELTs
Authors:Kellner, S.; Ragazzoni, R.; Diolaiti, E.; Gaessler, W.; Farinato, J.
Publisher:SPIE
Date of Publication (YYYY-MM-DD):2006
Title of Proceedings:Advances in Adaptive Optics II
Start Page:62725E-1
End Page:9
Title of Series:SPIE
Volume (in Series):6272
Name of Conference/Meeting:Advances in Adaptive Optics II
Audience:Not Specified
Abstract / Description:Laser Guide Star Adaptive Optics systems become in the moment reality at several 8...10m class telescope facilities. At these aperture diameters all effects, arising from the finite distance and vertical extend of the artificial excited guide star can still be neglected for the wavefront sensing process. This is changing completely when the telescope diameter become further increased as it is the case of next generation Extremely Large Telescopes. Effects such as perspective elongation become dominant and impact negatively the wavefront sensing process. This will result in severe quality restrictions for next generation Adaptive Optics systems. In this paper we want to introduce and explain in detail a novel kind of wavefront sensing techniques, optimized to overcome perspective elongation. Its basic idea is to project the generated LGS virtually to infinity. We will give a theoretical introduction and some background information about the proposed sensing concept and introduce a practical solution for a potential optical setup. The latter is based on inverting the so called Bessel Beam concept, producing diffraction less beam over a certain finite range. Furthermore we will characterize the new sensor type, compare the senor efficiency to alternative approaches and discuss finally both its advantages and disadvantages.
Comment of the Author/Creator:Date: 2006, July 1, 2006
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bi...
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.