Planetary, Solar and Heliospheric Radio Emissions (co-organized)
Convener: Patrick Galopeau  | Co-Convener: Mohammed Y. Boudjada 
Oral Programme
 / Fri, 07 May, 15:30–17:15  / Room 26
Poster Programme
 / Attendance Fri, 07 May, 13:30–15:00  / Hall XL
The session purpose is to discuss radiophysics progress in the study of non-thermal radio emissions emanating from the five magnetized planets, the Sun, the heliosphere, and extra-solar planets. Particular attention is given to observations and interpretations of radio wave phenomena, in particular those observed by ground radiotelescope or spacecraft experiments. Theoretical modelling, as well as radiophysics phenomena, are recommended especially for the comparative studies between magnetized planets, or among the Sun and the planets. New advances in the field of ground-based giant radiotelescopes (e.g. LOFAR, FASR) are supported with main emphasis on, one side, the development of new generation of radio reception system (antennas and instruments), and on other side the applied methods towards a synergy between space and ground-based stereoscopic observations. Further preparations, evaluations, investigations, analyses of forthcoming (e.g. Juno, Resonance, Solar Orbiter), actual (e.g. Cassini/RPWS, Stereo/SWAVES, Wind/WAVES) and previous (e.g. Voyager, Galileo, Ulysses) space missions are also encouraged.