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.; Withington, S.; Yassin, G.. - 14:(2005), pp. 245-250. (Intervento presentato al convegno Dome C Astronomy and Astrophysics Meeting tenutosi a 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.; Withington, S.; Yassin, G.. - 14:(2005), pp. 245-250. (Intervento presentato al convegno Dome C Astronomy and Astrophysics Meeting tenutosi a 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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