Practical beam transport for PFI

David Mozurkewich, John Young*, Michael Ireland

*Corresponding author for this work

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    2 Citations (Scopus)

    Abstract

    The Planet Formation Imager (PFI) is a future kilometric-baseline infrared interferometer to image the complex physical processes of planet formation. Technologies that could be used to transport starlight to a central beam-combining laboratory in PFI include free-space propagation in air or vacuum, and optical fibres. This paper addresses the design and cost issues associated with free-space propagation in vacuum pipes. The signal losses due to diffraction over long differential paths are evaluated, and conceptual beam transport designs employing pupil management to ameliorate these losses are presented and discussed.

    Original languageEnglish
    Title of host publicationOptical and Infrared Interferometry and Imaging V
    EditorsMichelle J. Creech-Eakman, Fabien Malbet, Peter G. Tuthill
    PublisherSPIE
    ISBN (Electronic)9781510601932
    DOIs
    Publication statusPublished - 2016
    EventOptical and Infrared Interferometry and Imaging V - Edinburgh, United Kingdom
    Duration: 27 Jun 20161 Jul 2016

    Publication series

    NameProceedings of SPIE - The International Society for Optical Engineering
    Volume9907
    ISSN (Print)0277-786X
    ISSN (Electronic)1996-756X

    Conference

    ConferenceOptical and Infrared Interferometry and Imaging V
    Country/TerritoryUnited Kingdom
    CityEdinburgh
    Period27/06/161/07/16

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