We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

SLODAR : measuring optical turbulence altitude with a Shack-Hartmann wavefront sensor.

Wilson, R. W. (2002) 'SLODAR : measuring optical turbulence altitude with a Shack-Hartmann wavefront sensor.', Monthly notices of the Royal Astronomical Society., 337 (1). pp. 103-108.


This paper discusses the use of Shack–Hartmann wavefront sensors to determine the vertical distribution of atmospheric optical turbulence above large telescopes. It is demonstrated that the turbulence altitude profile can be recovered reliably from time-averaged spatial cross-correlations of the local wavefront slopes for Shack–Hartmann observations of binary stars. The method, which is referred to as SLODAR, is analogous to the well known SCIDAR scintillation profiling technique, and a calibration against contemporaneous SCIDAR observations is shown. Hardware requirements are simplified relative to the scintillation method, and the number of suitable target objects is larger. The implementation of a Shack–Hartmann based turbulence monitor for use at the William Herschel Telescope is described. The system will be used to optimize adaptive optical observations at the telescope and to characterize anisoplanatic variations of the corrected point spread function.

Item Type:Article
Additional Information:
Keywords:Atmospheric effects, Instrumentation, Adaptive optics, Site testing, Telescopes.
Full text:Full text not available from this repository.
Publisher Web site:
Record Created:22 Nov 2006
Last Modified:08 Apr 2009 16:25

Social bookmarking: del.icio.usConnoteaBibSonomyCiteULikeFacebookTwitterExport: EndNote, Zotero | BibTex
Look up in GoogleScholar | Find in a UK Library