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Cryogenic Integration of the 2-14 GHz Eleven Feed in a Wideband Receiver for VLBI2010The next generation VLBI systems require the design of a wideband receiver covering the 2-14 GHz range, necessitating a wideband feed. Presented here are the 2009 development of a cryogenic 2-14 GHz Eleven feed for reflector radio telescope antennas, including its integration into a cryogenic receiver. The Eleven feed is designed for dual linear polarization and consists of four log-periodic folded dipole arrays. Each pair of arrays is fed by a differential two-wire transmission line connected either to balun or a differential LNA. The present configuration has been measured in many configurations, at various independent labs - corresponding simulations have been done. The results show (across the band) a high polarization efficiency for the feed, with a nearly constant beam width, a reflection coefficient below -10dB, and a constant phase center. Electrical parameters under cryogenic conditions and measured receiver noise temperatures are presented.
Document ID
20110011804
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Pantaleev, Miroslaw
(Onsala Space Observatory Sweden)
Jang, Jian
(Chalmers Univ. of Technology Goeteborg, Sweden)
Karadikar, Yogesh
(Chalmers Univ. of Technology Goeteborg, Sweden)
Helldner, Leif
(Onsala Space Observatory Sweden)
Klein, Benjamin
(Hartebeesthoek Radio Astronomy Observatory Johannesburg, South Africa)
Haas, Rudiger
(Onsala Space Observatory Sweden)
Zaman, Ashraf
(Chalmers Univ. of Technology Goeteborg, Sweden)
Zamani, Mojtaba
(Chalmers Univ. of Technology Goeteborg, Sweden)
Kildal, Per-Simon
(Chalmers Univ. of Technology Goeteborg, Sweden)
Date Acquired
August 25, 2013
Publication Date
December 1, 2010
Publication Information
Publication: Proceedings of the Sixth General Meeting of the International VLBI Service for Geodesy and Astrometry
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Public Use Permitted.
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