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
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.
