Distributed H∞ Control of Segmented Telescope Mirrors

dc.contributor.authorUlutas, Baris
dc.contributor.supervisorSuleman, Afzal
dc.contributor.supervisorPark, Edward Jung Wook
dc.date.accessioned2014-08-12T22:38:23Z
dc.date.available2014-08-12T22:38:23Z
dc.date.copyright2014en_US
dc.date.issued2014-08-12
dc.degree.departmentDepartment of Mechanical Engineering
dc.degree.levelDoctor of Philosophy Ph.D.en_US
dc.description.abstractSegmented mirrors are to be used in the next generation of the ground-based optical telescopes to increase the size of the primary mirrors. A larger primary mirror enables the collection of more light, which results in higher image resolutions. The main reason behind the choice of segmented mirrors over monolithic mirrors is to reduce manufacturing, transportation, and maintenance costs of the overall system. However, segmented mirrors bring new challenges to the telescope design and control problem. The large number of inputs and outputs make the computations for centralized control schemes intractable. Centralized controllers also result in systems that are vulnerable to a complete system failure due to a malfunction of the controller. Distributed control is a viable alternative that requires the use of a network of simple individual segment controllers that can address two levels of coupling among segments and achieve the same performance objectives. Since segments share a common support structure, there exists a coupling among segments at the dynamics level. Any control action in one segment may excite the natural modes of the support structure and disturb other segments through this common support. In addition, the objective of maintaining a smooth mirror surface requires minimization of the relative displacements among neighbouring segment edges. This creates another level of coupling generally referred to as the objective coupling. This dissertation investigates the distributed H∞ control of the segmented next generation telescope primary mirrors in the presence of wind disturbances. Three distributed H∞ control techniques are proposed and tested on three segmented primary mirror models: the dynamically uncoupled model, the dynamically coupled model and the finite element model of Thirty Meter Telescope (TMT) project. It is shown that the distributed H∞ controllers are able to satisfy the stringent imaging performance requirements.en_US
dc.description.proquestcode0548en_US
dc.description.scholarlevelGraduateen_US
dc.identifier.bibliographicCitationB. Ulutas, E.J. Park, A. Suleman, Distributed and centralized H∞ control of large segmented telescopes, Proceedings of ASME International Mechanical Engineering Congress and Exposition, Vancouver, BC, (2010) 1129-1137.en_US
dc.identifier.bibliographicCitationB. Ulutas, E.J. Park, A. Suleman, Decomposition-based distributed H∞ control of large segmented telescopes, Proceedings of CSME International Congress, Toronto, ON, (2014).en_US
dc.identifier.bibliographicCitationB. Ulutas, D. Kerley, J. Dunn, A. Suleman, E.J. Park, Distributed H∞ control of dynamically coupled segmented telescope mirrors: Design and simulation, Mechatronics, 22(1) (2012) 121-135.en_US
dc.identifier.bibliographicCitationB. Ulutas, E.J. Park, A. Suleman, LMI-based Distributed H∞ control of dynamically coupled large segmented telescope mirrors, Proceedings of IEEE/ASME International Conference on Advanced Intelligent Mechatronics, Besancon, France, (2014).en_US
dc.identifier.urihttp://hdl.handle.net/1828/5550
dc.languageEnglisheng
dc.language.isoenen_US
dc.rights.tempAvailable to the World Wide Weben_US
dc.subjectrobust controlen_US
dc.subjectH∞ controlen_US
dc.subjectdistributed controlen_US
dc.subjectsegmented mirroren_US
dc.subjectnext generation telescopeen_US
dc.subjectactive opticsen_US
dc.titleDistributed H∞ Control of Segmented Telescope Mirrorsen_US
dc.typeThesisen_US

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