Fig. 3From: Ellerman bombs observed with the new vacuum solar telescope and the atmospheric imaging assembly onboard the solar dynamics observatoryLeft panel: scatter plot depicting the relationship between the intensity and lifetime of EBs identified from the Hα wing images. Right panel: scatter plot depicting the relationship between EB intensity in Hα wing and AIA 1700 Å images. Each red diamond represents the average 1700 Å intensity in each bin of Hα wing intensity. Red lines represent the results from a linear fittingBack to article page