dc.creatorSERGIO VAZQUEZ Y MONTIEL
dc.date2011-05-01
dc.date.accessioned2023-07-25T16:24:06Z
dc.date.available2023-07-25T16:24:06Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1665
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806859
dc.descriptionIn this paper, an optical design is presented for an anastigmatic telescope with back focal length corrected with exact ray tracing to eliminate spherical, coma, and astigmatism aberrations. The telescope is formed of three conical mirrors, two of them polished on the same substratum. The optical design is divided into three stages: we began the design obtaining the Gaussian parameters in a first-order solution; posteriorly, were obtained analytically the three mirrors’ asphericity in a third-order design. The final design stage consists of the implementation of the Fermat’s principle, the Abbe sine condition, and the Coddingtonequations for the exact correction for the three aforementioned aberrations. © 2011 Optical Society of America
dc.formatapplication/pdf
dc.languageeng
dc.publisherApplied Optics
dc.relationcitation:Herrera, J., et al., (2011), Variant of the anastigmatic telescope with three mirrors for back focal length, Applied Optics. Vol. 50(13):1905-1914
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Anastigmatic telescope/Anastigmatic telescope
dc.subjectinfo:eu-repo/classification/Back focal length/Back focal length
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/22
dc.subjectinfo:eu-repo/classification/cti/2209
dc.subjectinfo:eu-repo/classification/cti/2209
dc.titleVariant of the anastigmatic telescope with three mirrors for back focal length
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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