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Simultaneous radio and extreme ultraviolet (EUV)/white-light imaging data areexamined for a solar type II radio burst occurring on 2010 March 18 to deduceits source location. Using a bow-shock model, we reconstruct the 3-dimensionalEUV wave front (presumably the type-II emitting shock) based on the imagingdata of the two STEREO spacecraft. It is then combined with the Nan\c{c}ayradio imaging data to infer the 3-dimensional position of the type II source.It is found that the type II source coincides with the interface between theCME EUV wave front and a nearby coronal ray structure, providing evidence thatthe type II emission is physically related to the CME-ray interaction. Thisresult, consistent with those of previous studies, is based on simultaneousradio and EUV imaging data for the first time.

A solar type II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging