Putting It All Together
•FASR
•Map coronal field strength in active regions
•Image type III bursts and other emissions to obtain acceleration site and trajectory to 1.5 Rsun
•Image CMEs, and equivalent of EIT waves.
•Image some coronal type II bursts
•LOFAR (or FASR if not co-located)
•Image type III bursts to obtain trajectory to 2.5 Rsun (possible limitation on frequency coverage) •Image coronal type II bursts and associated nonthermal emission to 2.5 Rsun