Institute of Astronomy
Radio Astronomy and Plasma Physics Group
Eidgenössische Technische Hochschule Zürich
Swiss Federal Institute of Technology,  Zürich
          
Conclusions (Cont.)
- The location of the decimetric emission (looptop, footpoint, reconnection region, cusp, shock etc.) will help to clarify the emission process. The coronal context is given by EUV, HXR and SXR observations.
- Even if it does not occur in every flare, the coherent radio emission will have a  great diagnostic value for particle acceleration, shocks and particle propagation in flares.
- FASR will be the only instrument that has sufficient frequencies in the decimeter range to identify the emission process like a spectrometer.
- FASR will be able to trace back type II and III bursts to their origin.