Antenna Design and Distribution for a LOFAR Super Station in Nançay

J. N. Girard; P. Zarka; M. Tagger; L. Denis; D. Charrier; A. Konovalenko

doi:doi:10.1553/PRE7s495

H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)

Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

Helmut Rucker
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

William Kurth
Department of Physics and Astronomy, University of Iowa, Iowa City, USA

Philippe Louarn
Centre d'Etude Spatiale de Rayonnements, CNRS/Universitè Paul-Sabatier Toulouse III, Toulouse, France

Georg Fischer
Space Research Institute, Austrian Academy of Sciences, Graz, Austria

ISBN 978-3-7001-7125-6 Print Edition
ISBN 978-3-7001-7246-8 Online Edition

doi: https://doi.org/10.1553/PRE7

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The 7th International Workshop on "Planetary, Solar and Heliospheric Radio Emissions" is the continuation of an established tradition: This PRE VII conference followed previous successful international workshops held at Graz, Austria, in 1984, 1987, 1991, 1996, 2001, and 2005. This 7th workshop in September 2010 offered again the unique opportunity to discuss the observations from Cassini at Saturn and to investigate the measurements by other spacecraft and from the ground of the Jovian, terrestrial and solar radio emissions, also including studies on radiation from exoplanetary sources.

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Antenna Design and Distribution for a LOFAR Super Station in Nançay

J. N. Girard,

P. Zarka,

M. Tagger,

L. Denis,

D. Charrier,

A. Konovalenko

Planetary Radio Emissions VII, pp. 495-504, 2011/12/28

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

doi: 10.1553/PRE7s495

€ 79,–

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doi:10.1553/PRE7s495

Abstract

The Nançay radio astronomy observatory and associated laboratories are developing the concept of a “Super Station” for extending the LOFAR station now installed and operational in Nan¸cay. The LOFAR Super Station (LSS) will increase the number of high sensitivity long baselines, provide short baselines and an alternate core, and be a large standalone instrument. It will operate in the low frequency band of LOFAR (30–80 MHz) and extend this range to lower frequencies. Three key developments for the LSS are described here: (i) the design of a specific antenna, and the distribution of such antennas (ii) at small-scale (analog-phased mini array) and (iii) at large-scale (the whole LSS).

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Published Online: 2011/12/28 16:34:11

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H.O. Rucker - W.S. Kurth - P. Louarn - G. Fischer (Eds.)

Planetary Radio Emissions VII

Proceedings of the 7th International Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Graz, Austria, September 15–17, 2010

Antenna Design and Distribution for a LOFAR Super Station in Nançay

€ 79,–

Abstract