CLOVER experiment: The receiver block

G. Pisano, P. A R Ade, C. Calderon, A. D. Challinor, P. De Bernardis, L. Dunlop, W. K. Gear, Y. Giraud-Héraud, D. J. Goldie, K. J B Grainge, K. G. Isaak, B. Johnson, M. E. Jones, A. N. Lasenby, B. Maffei, P. D. Mauskopf, S. J. Melhuish, A. Orlando, L. Piccirillo, A. C. TaylorS. Withington, G. Yassin

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


    The ClOVER instrument (described elsewhere in this volume) is being built to measure the B-mode polarisation of the Cosmic Microwave Background. Each of the 256 pixels is made up a pseudo-correlation receiver that can be realised using either waveguide or microstrip technology. In this work we present a design study for a possible waveguide-based solution. Each of the individual components has been optimised using electromagnetic finite-element modelling software (HFSS). © EAS, EDP Sciences 2005.
    Original languageEnglish
    Title of host publicationEAS Publications Series|EAS Publ. Ser.
    Number of pages5
    Publication statusPublished - 2005
    EventDome C Astronomy and Astrophysics Meeting - Toulouse
    Duration: 1 Jul 2005 → …

    Publication series

    NameEAS Publications Series


    ConferenceDome C Astronomy and Astrophysics Meeting
    Period1/07/05 → …


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