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.
|Name||EAS Publications Series|
|Conference||Dome C Astronomy and Astrophysics Meeting|
|Period||1/07/05 → …|