159 articles – 2000 Notices  [english version]
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Dome C Astronomy and Astrophysics Meeting, Toulouse : France (2004)
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-Héraud1, 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. Taylor, S. Withington, G. Yassin

The C$_{\it l}$OVER 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).
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
APC - Cosmologie et Gravitation
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique