Fig. 4From: Ellerman bombs observed with the new vacuum solar telescope and the atmospheric imaging assembly onboard the solar dynamics observatoryDistributions of the intensities of EBs in the Hα wing images, the AIA 1700 Å intensities at the locations of EBs, and the lifetimes of EBs derived from Hα wing observations. The red and blue histograms represent the results for the BP-related EBs and EBs that are not related to BPs, respectivelyBack to article page