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Figure 3 | Earth, Planets and Space

Figure 3

From: How does ionospheric TEC vary if solar EUV irradiance continuously decreases?

Figure 3

The TEC values at the zero solar EUV point. The left column is the TEC extrapolated from the linear TEC-EUV fitting for which the data of EUV < 4 were used (see Figure 2a), and the right column is the TEC extrapolated from the quadratic TEC-EUV fitting for which the data of the full EUV range were used (see Figure 2b). The white lines denote the dip equator, and the black contours denote zero TEC.

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