Butterley, T. and Love, G. D. and Wilson, R. W. and Myers, R. M. and Morris, T. J. (2006) 'A Shack-Hartmann wavefront sensor projected on to the sky with reduced focal anisoplanatism.', Monthly notices of the Royal Astronomical Society., 368 (2). pp. 837-843.
A method for producing a laser guide star wavefront sensor for adaptive optics with reduced focal anisoplanatism is presented. A theoretical analysis and numerical simulations have been carried out and the results are presented. The technique, named Sky-Projected Laser Array Shack–Hartmann (SPLASH), is shown to suffer considerably less from focal anisoplanatism than a conventional laser guide star system. The method is potentially suitable for large telescope apertures (8 m), and possibly for extremely large telescopes.
|Keywords:||Instrumentation, Adaptive optics, Telescopes.|
|Full text:||(NA) Not Applicable |
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|Publisher Web site:||http://dx.doi.org/10.1111/j.1365-2966.2006.10160.x|
|Publisher statement:||The definitive version is available at www.blackwell-synergy.com|
|Record Created:||02 May 2008|
|Last Modified:||16 Aug 2011 09:26|
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