Solar Observations with LOFAR

G. Mann; C. Vocks; F. Breitling

doi:doi:10.1553/PRE7s507

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

2011 578 Seiten, 23x15cm, broschiert
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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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Solar Observations with LOFAR

G. Mann,

C. Vocks,

F. Breitling

Planetary Radio Emissions VII, pp. 507-512, 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/PRE7s507

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doi:10.1553/PRE7s507

Abstract

The LOw Frequency ARray (LOFAR) is a novel radio telescope that consists of 20 core stations near Exloo in the Netherlands, 18 Dutch remote stations, and 8 international stations all distributed over central Europe. One of them was built in Potsdam. LOFAR is a radio interferometer for the frequency range of 30-240 MHz and will exceed the sensitivity and resolution of existing instruments by more than one order of magnitude. ”Solar Physics and Space Weather with LOFAR” is one of LOFAR’s Key Science Projects. Since LOFAR is working in the frequency range of 30-240 MHz, it is able to deliver radio images of the Sun. The solar radio radiation in this frequency range is emitted from the outer corona. Since radio waves are strongly scattered in the corona, the angular resolution of LOFAR’s radio maps will be limited to a few 10 arcseconds. The necessary baselines include the core and the nearest remote stations.

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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

Solar Observations with LOFAR

€ 79,–

Abstract