Fig. 3From: Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flaresTEC simulated by GAIA model. The TEC distributions for RUN-Fd, RUN-Ff, RUN-FS35, RUN-FS15, and RUN-FS10 at 130°E, where, locally, at the time of the flare are around noon for the X1.1-class flare on November 8, 2013Back to article page