Conference item icon

Conference item

Clover experiment: The receiver block

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).
Publication status:
Published

Actions

Access Document

Publisher copy:
10.1051/eas:2005038

Authors


Journal:
Dome C: Astronomy and Astrophysics Meeting More from this journal
Volume:
14
Pages:
245-250
Publication date:
2005-01-01
Event title:
Dome C Astronomy and Astrophysics Meeting
DOI:
EISSN:
1638-1963
ISSN:
1633-4760
ISBN:
2868838359


Pubs id:
pubs:18877
UUID:
uuid:eda0ab6a-b8b1-4882-ae8b-150be91b71d4
Local pid:
pubs:18877
Source identifiers:
18877
Deposit date:
2012-12-19
ARK identifier:

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP