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 contribution

Abstract

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).

Original languageEnglish (US)
Title of host publicationProceedings - CIS Workshops 2007, 2007 International Conference on Computational Intelligence and Security Workshops, CISW 2007
Pages245-250
Number of pages6
DOIs
StatePublished - 2005
EventDome C Astronomy and Astrophysics Meeting - Toulouse, France
Duration: Jun 28 2004Jun 30 2004

Publication series

NameEAS Publications Series
Volume14
ISSN (Print)1633-4760
ISSN (Electronic)1638-1963

Other

OtherDome C Astronomy and Astrophysics Meeting
CountryFrance
CityToulouse
Period6/28/046/30/04

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Engineering(all)
  • Space and Planetary Science

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