Imaging spectroscopy of the 2002 Mar 14 flare.  
Images and spectra from RHESSI are compared with Nobeyama images and
spectra (M. Kundu), with discussion of the radio evidence for a very hot
(~60 MK) thermal source not seen by RHESSI.  Electron energetics are
derived in two different ways from RHESSI spectra: parametric fits to
photon spectra and forward fits from electron thick-target parameters. 
The similarities and differences will be compared.