SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO

T. Nikola, G. J. Stacey, T. E. Oberst, S. C. Parshley, A. A. Stark, N. Tothill, J. Harnett

    Research output: Chapter in Book / Conference PaperConference Paper

    Abstract

    ![CDATA[The South Pole Imaging Fabry-Perot Interferometer, SPIFI, is a direct detection imaging spectrometer for submillimeter astronomy in the telluric windows at 200 pm, 350 m, and 450 pm that are available at the South Pole (B1, B2). The main components of SPIFI are the cryogenic Fabry-Perot interferometers (FPI's) which can be tuned to any wavelength within the atmospheric windows and the detector array which provides a two dimensional field of view.]]
    Original languageEnglish
    Title of host publicationProceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts
    PublisherNational Radio Astronomy Observatory
    Pages357-364
    Number of pages8
    Publication statusPublished - 2004
    EventInternational Symposium on Space Terahertz Technology -
    Duration: 1 Jan 2008 → …

    Conference

    ConferenceInternational Symposium on Space Terahertz Technology
    Period1/01/08 → …

    Fingerprint

    Dive into the research topics of 'SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO'. Together they form a unique fingerprint.

    Cite this