Key topis of this session are the recent developments in the study of
non-thermal radio emissions from the Sun, the five radio planets, and
potential radio emissions from exoplanets. Special emphasis is put on
current missions like Cassini and STEREO, but also new findings from
data of older missions (Voyager, Galileo, Wind, Ulysses) and ground-
based observations are welcome. Presentations should focus on physical
properties of radio emissions like rotational modulation, fine
structures in dynamic spectra, polarization as well as source
direction, and theorectical modeling and simulation of plasma and
magnetic processes leading to their generation. Key question for
potential future missions like Juno, Solar Orbiter or Laplace can also
be addressed. New developments in ground-based radio telescopes (e.g.
LOFAR, FASR) will be matters of discussion, that should lead to a
better coordination of ground- and space-based observations. Oral as
well as poster presentations are welcome.