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A telescope made with cylinders - I. Some analytical results

dc.contributor.authorBalasubramanyam, R
dc.date.accessioned2007-02-07T11:27:02Z
dc.date.available2007-02-07T11:27:02Z
dc.date.issued2004-11
dc.descriptionRestricted Access.en
dc.description.abstractA novel optical design for a telescope, especially suited for constructing large telescopes at submillimetre to optical wavelengths, was proposed recently. In this paper, we present some analytical results related to such novel optics. We show that, for oblique incidence, the line focus of a parabolic cylinder merely shifts by the same angle in the opposite direction. We also derive the equation defining the shape of the mirror that converts a cylindrical wavefront to a spherical wavefront.en
dc.format.extent8338 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2004, Vol.354, Issue 4, p1189-1193.en
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/2289/2078
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004MNRAS.354.1189B&link_type=ARTICLE&db_key=ASTen
dc.rights2004 Royal Astronomical Societyen
dc.subjectinstrumentation: miscellaneousen
dc.subjectmethods: analyticalen
dc.subjecttelescopesen
dc.subjectsubmillimetreen
dc.titleA telescope made with cylinders - I. Some analytical resultsen
dc.typeArticleen

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