DocumentCode
284207
Title
The new L/K-band polarimeter system for the 32 m radiotelescope at Cambridge
Author
Ludke, E. ; Roddis, N. ; Davis, R.J. ; Battilana, J.A.
Author_Institution
Nuffield Radio Astron. Lab., Jodrell Bank, UK
fYear
1993
fDate
1993
Firstpage
610
Abstract
A new 32 m Cassegrain radio telescope has been added to Jodrell Bank´s MERLIN network. For wavelengths of 6 cm and less, conical corrugated feed horns have been employed with excellent results, both in terms of aperture efficiency and system noise temperature. Furthermore such feeds perform well in the reception of circularly polarized waves, an essential requirement for MERLIN. A low-cost alternative to the conical corrugated horn has been sought. The `diagonal horn´ was identified as a possible candidate and investigations have been carried out into its suitability as a low-cost 20 cm horn, using scale models at 6 cm and 1.3 cm wavelengths. The authors describe the diagonal horn design and polarization characteristics and compare the radiotelescope performance at 6 cm with diagonal and corrugated horns
Keywords
antenna feeders; astronomical polarimetry; electromagnetic wave polarisation; horn antennas; radiotelescopes; reflector antennas; 1.3 cm; 6 cm; Cambridge; Cassegrain radio telescope; EHF; Jodrell Bank; L/K-band polarimeter system; MERLIN network; SHF; aperture efficiency; circularly polarized waves; conical corrugated feed horns; diagonal horn; noise temperature; polarization characteristics; radiotelescope;
fLanguage
English
Publisher
iet
Conference_Titel
Antennas and Propagation, 1993., Eighth International Conference on
Conference_Location
Edinburgh
Print_ISBN
0-85296-572-9
Type
conf
Filename
224678
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