Fig. 4From: Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flaresRatio of TEC distribution calculated by GAIA. The ratio of TEC distribution calculated by RUN-Fd for RUN-Ff, RUN-FS35, RUN-FS15, and RUN-FS10 at 130°E around noon local time at the time of the flare shown in Fig. 3 for the X1.1-class flare on November 8, 2013Back to article page