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    Radio Properties of the Auroral ionosphere, Supplement to Final Report (Phase I)

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    GI Reports 103.pdf
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    Author
    Reid, G. C.
    Stiltner, E.
    Metadata
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    URI
    http://hdl.handle.net/11122/3599
    Abstract
    The usefulness of the phase-sweep technique in interferometers designed to record radio star signals is discussed. Interferometers of this type have been built for use at frequencies of 223 and 456 Mcs., and their electronic design is explained in some detail. The report also includes a discussion of the automatic data processing system which has been designed to operate in conjunction with the interferometers in the analysis of the amplitude scintillation of radio stars.
    Table of Contents
    List of Figures -- Abstract -- Introduction -- Total Power Interferometer -- Phase-Sweep Interferometer -- 223 Mes. Equipment : Circuit description ; Mixers ; Phase-lock control unit ; IP amplifier ; Tuned audio amplifier ; DC amplifier ; Auxiliary equipment -- 456 Mes. Equipment -- Digitizing Equipment -- Calculation of Mean Power Fluctuation -- Acknowledgements -- References -- Figures
    Date
    1960-02-01
    Source
    Geophysical Institute
    Publisher
    Geophysical Institute at the University of Alaska
    Type
    Report
    Peer-Reviewed
    Yes
    Collections
    GI Reports

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