Description: Remote sensing of Solar System objects such as planetary atmospheres, comets and asteroids, or the space between them, relies largely on the analysis of the solar light scattered by dust particles and clouds. Polarization is an invaluable tool for obtaining information on the physical properties (size, shape, and composition) and location of the scattering particles in the corresponding atmosphere.
The aim of this session is to bring together observers, modelers, and experimental physicists to discuss the most recent results and advances in the characterization of dust particles by their spectro-polarimetric pattern.