Fig. 1
Dynamic radio spectrograms and lightcurves of radio, soft, and hard X-ray emissions during the 3 November 2010 eruptive event. Solar radio flux density measured by the telescope in San Vito (RSTN) at 245 MHz is divided by a factor of ten for clarity. The vertical dashed line indicates the peak time (12:14:00 UT) of the hard X-ray and microwave bursts.
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