Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6015
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dc.contributor.authorBanyal, R. K-
dc.contributor.authorRavindra, B-
dc.contributor.authorChatterjee, S-
dc.date.accessioned2013-03-14T10:35:07Z-
dc.date.available2013-03-14T10:35:07Z-
dc.date.issued2013-03-25-
dc.identifier.citationOptics Express, Vol. 21, No. 6, pp. 7065-7081en
dc.identifier.issn1559-128X-
dc.identifier.urihttp://hdl.handle.net/2248/6015-
dc.descriptionRestricted Accessen
dc.description.abstractIn this paper, an opto-thermal analysis of a moderately heated lightweighted solar telescope mirror is carried out using 3D finite element analysis (FEA). A physically realistic heat transfer model is developed to account for the radiative heating and energy exchange of the mirror with surroundings. The numerical simulations show the non-uniform temperature distribution and associated thermo-elastic distortions of the mirror blank clearly mimicking the underlying discrete geometry of the lightweighted substrate. The computed mechanical deformation data is analyzed with surface polynomials and the optical quality of the mirror is evaluated with the help of a ray-tracing software. The thermal print-through distortions are further shown to contribute to optical figure changes and mid-spatial frequency errors of the mirror surface. A comparative study presented for three commonly used substrate materials, namely, Zerodur, Pyrex and Silicon Carbide (SiC) is relevant to vast area of large optics requirements in ground and space applications.en
dc.language.isoenen
dc.publisherOptical Society of Americaen
dc.relation.urihttp://dx.doi.org/10.1364/OE.21.007065en
dc.relation.urihttp://arxiv.org/abs/1302.6600en
dc.rights© Optical Society of Americaen
dc.subjectOptical design and fabricationen
dc.subjectTelescopesen
dc.subjectMirroren
dc.subjectThermal effectsen
dc.subjectOptical materialsen
dc.subjectAberration expansionsen
dc.titleOpto-thermal analysis of a lightweighted mirror for solar telescopeen
dc.typeArticleen
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