| The source was distinguished by its departure from the Neupert Effect - hard X-rays peaked late, and were much brighter than expected. |
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| The hard X-ray source matched the position of a compact microwave source judged to be free-free emission. |
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| The source exhibited an outward motion unprecedented for a hard X-ray source, and one which matched the motion of the unusual microwave source. The moving structures were embedded within a CME and (arguably) were associated with erupting filament material. | 
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| The moving hard X-ray/microwave source coincided with a slow-drift decimetric source that preceded the associated Type II (?) burst. |  |