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.

CLOVER experiment: The receiver block / Pisano, G., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., Gear, W.K., Giraud-Heraud, Y., Goldie, D.J., Grainge, K.J.B., Isaak, K.G., Johnson, B., Jones, M.E., Lasenby, A.N., Maffei, B., Mauskopf, P.D., Melhuish, S.J., Orlando, A., Piccirillo, L., Taylor, A.C., et al.. - 14:(2005), pp. 245-250. (Dome C Astronomy and Astrophysics Meeting Toulouse, fra ) [10.1051/eas:2005038].

CLOVER experiment: The receiver block

Pisano G.;De Bernardis P.;
2005

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). © EAS, EDP Sciences 2005.
2005
Dome C Astronomy and Astrophysics Meeting
Polarimetry, millimetre waves, microwave receivers, polarization modulation, Cosmic Microwave Background radiation
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
CLOVER experiment: The receiver block / Pisano, G., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., Gear, W.K., Giraud-Heraud, Y., Goldie, D.J., Grainge, K.J.B., Isaak, K.G., Johnson, B., Jones, M.E., Lasenby, A.N., Maffei, B., Mauskopf, P.D., Melhuish, S.J., Orlando, A., Piccirillo, L., Taylor, A.C., et al.. - 14:(2005), pp. 245-250. (Dome C Astronomy and Astrophysics Meeting Toulouse, fra ) [10.1051/eas:2005038].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1557174
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