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Evaluation of statistical turbulence models for use in the Distributed Kalman Filter

dc.contributor.authorCranney, Jesse
dc.contributor.authorPiatrou, Piotr
dc.contributor.authorDe Dona, Jose
dc.contributor.authorRigaut, Francois
dc.contributor.authorKorkiakoski, Visa
dc.contributor.editorDaniel, K
dc.coverage.spatialTenerife, Canary Islands, Spain
dc.date.accessioned2024-07-24T01:08:26Z
dc.date.available2024-07-24T01:08:26Z
dc.date.createdJune 25-30 2017
dc.date.issued2017
dc.date.updated2023-12-24T07:15:46Z
dc.description.abstractThe Kalman Filter (KF) application to wavefront control in Adaptive Optics (AO) shows great promise with respect to achieving the best atmospheric turbulence error rejection, provided an adequate model for the turbulence temporal dynamics exists. The advent of the computationally efficient Distributed Kalman Filter (DKF) algorithm makes the KF approach especially attractive for the future of high DOF AO systems (As is the case in the Extremely Large Telescope class). In this work we try to address a significant drawback of the existing DKF state space model, which is too simplistic (single parameter scalar diagonal state matrix) to describe the atmosphere turbulence dynamics. We investigate a broader family of Block-Toeplitz with Toeplitz Blocks (BTTB) state matrices, which, on one hand, are able to better grasp statistical properties of the turbulence to provide significantly better prediction power and, on the other hand, preserve the shift invariance property, a corner stone of the DKF algorithm. We demonstrate the capabilities of the new model in the end-to-end simulations of the DKF-driven Single Conjugate AO system.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.urihttps://hdl.handle.net/1885/733714163
dc.language.isoen_AUen_AU
dc.publisherInstituto de Astrofisica de Canarias
dc.relation.ispartofseries5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017
dc.rights© 2017 Instituto de Astrofisica de Canarias
dc.sourceAdaptive Optics for Extremely Large Telescopes, 2017 AO4ELT5
dc.titleEvaluation of statistical turbulence models for use in the Distributed Kalman Filter
dc.typeConference paper
local.bibliographicCitation.lastpage12
local.bibliographicCitation.startpage1
local.contributor.affiliationCranney, Jesse, College of Science, ANU
local.contributor.affiliationPiatrou, Piotr, College of Science, ANU
local.contributor.affiliationDe Dona, Jose, University of Newcastle
local.contributor.affiliationRigaut, Francois, College of Science, ANU
local.contributor.affiliationKorkiakoski, Visa, College of Science, ANU
local.contributor.authoruidCranney, Jesse, u1093816
local.contributor.authoruidPiatrou, Piotr, u5124553
local.contributor.authoruidRigaut, Francois, u5090915
local.contributor.authoruidKorkiakoski, Visa, u1025408
local.description.embargo2099-12-31
local.description.notesImported from ARIES
local.description.refereedNo
local.identifier.absfor510102 - Astronomical instrumentation
local.identifier.absseo280120 - Expanding knowledge in the physical sciences
local.identifier.ariespublicationa383154xPUB31681
local.identifier.doi10.26698/AO4ELT5.0087
local.identifier.scopusID2-s2.0-85049209799
local.type.statusPublished Version

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