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A new member of the growing family of magnetars, i.e., SGR 1935+2154 was discovered by Swift on July 05, 2014 via detection of persistent short duration bursts of X-rays. The source was active during 2015-2016 years that is well documented by Swift, GBM (Fermi), RHESSI and Konus-Wind detections. Lomonosov has joined the study of the new magnetar activity by detecting 14 flashes from this SGR 1935+2154 during 2016. New and already known types of flashes are revealed by the BDRG detector that is flying on-board of Lomonosov satellite. Characteristics of detected flashes and their specific role in understanding of the soft gamma repeater flaring mechanism will be discussed in this presentation.