• 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

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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
€  79,–   

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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.

Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
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Planetary Radio Emissions VII


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



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Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
A-1011 Wien, Dr. Ignaz Seipel-Platz 2,
Tel. +43-1-515 81/DW 3420, Fax +43-1-515 81/DW 3400
https://verlag.oeaw.ac.at, e-mail: bestellung.verlag@oeaw.ac.at
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Solar Radio Emissions in View of the Solar Orbiter Mission (invited; abstract)

    M. Maksimovic

Planetary Radio Emissions VII, pp. 417-418, 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/PRE7s417

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doi:10.1553/PRE7s417


Abstract

One of the science goals of the Solar Orbiter mission is to study the connectivitybetween the solar corona and the inner Heliosphere as close as from 0.3 AU. Withthis respect the study of Solar radio emissions produced energetic electrons eitherflare or shock accelerated will be of prime importance. I will first review some recentfindings obtained with the help of Ulysses, WIND and Stereo observations. I willthen present the expected capabilities of the Solar Orbiter instrumentation relevantto the discussed topic.

Published Online: 2011/12/28 15:37:07

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