Advancing Radio Diagnostics of Space Weather Plasma Processes

Abstract

Space Weather perturbations are originated by a variety of plasma processes, whose signatures are observable in the radio spectrum. The interpretation of these signatures to infer the physics at the sources is a fundamental requirement in developing Space Weather science and operation models. Hence, the advancement both of radio observation techniques and radio emission and propagation modelling is a must. A step to achieve this goal cannot be separated from the availability of a collaborative approach for data and model sharing and reviewing.