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Solar hard X-ray and gamma-emission was measured by BDRG instrument, the part of set of instruments operated onboard Russian satellite Lomonosov from April 2016 till now (solar-synchronous orbit with altitude 490 km, inclination of 97.6 degrees). Lomonosov measurements (14 flares with the X-ray energy > 10 keV, and more than half of them have class in Soft X-Rays less than C2) were compared to the data obtained with RHESSI, Konus-Wind, Fermi observatory, Radio Solar Telescope Net (RSTN) and with the Nobeyama Radioheliograph (NoRH) operating at the same time. The quasi-periodicities with different periods were found in some of them.