This work proposes to study the impact of GLE induced by Extreme Solar Flares on the SER for flights representative to the world-air traffic. A GLE physical model was confronted to cosmic ray variations measured with neutron monitors during the GLEs 5 and 69. Based on said GLE physical model and SEU occurrence models, investigations were performed to assess the SER during these GLEs for a bulk 90-nm SRAM COTS SRAM. The main conclusion is that the GLE impact must be considered in the risk assessment, which requires a physical description of the additional solar cosmic rays and a realistic consideration of the air traffic.