Fig. 1.
Moving radio bursts associated with the expansion of the 22 May 2013 CME in the solar corona. NRH radio contours at 150.9 MHz (orange) and 173.2 MHz (green) are overlaid on AIA 211 Å running-difference images in each panel. Three moving radio bursts were identified and labelled as Source 1 (top panels), Source 2 (middle panels), and Source 3 (bottom panels). The AIA images show the evolution of the CME through time.
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