Modeling the adaptive optics systems on the Giant Magellan Telescope

Marcos A. Van Dam, Philip M. Hinz, Johanan L. Codona, Michael Hart, Aurea Garcia-Rissmann, Matt W. Johns, Stephen A. Shectman, Antonin H. Bouchez, Brian A. McLeod, Francois Rigaut

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

9 Citations (Scopus)

Abstract

Modeling adaptive optics (AO) systems is crucial to understanding their performance and a key aid in their design. The Giant Magellan Telescope (GMT) is planning three AO modes at first light: natural guide star AO, ground-layer AO and laser tomography AO. This paper describes how a modified version of YAO, an open-source general-purpose AO simulation tool written in Yorick, is used to simulate the GMT AO modes. The simulation tool was used to determine the piston segment error for the GMT. In addition, we present a comparison of different turbulence simulation approaches.

Original languageEnglish
Title of host publicationAdaptive Optics Systems II
EditionPART 1
DOIs
Publication statusPublished - 2010
Externally publishedYes
EventAdaptive Optics Systems II - San Diego, CA, United States
Duration: 27 Jun 20102 Jul 2010

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
NumberPART 1
Volume7736
ISSN (Print)0277-786X

Conference

ConferenceAdaptive Optics Systems II
Country/TerritoryUnited States
CitySan Diego, CA
Period27/06/102/07/10

Fingerprint

Dive into the research topics of 'Modeling the adaptive optics systems on the Giant Magellan Telescope'. Together they form a unique fingerprint.

Cite this