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Fig. 4 | Earth, Planets and Space

Fig. 4

From: On using a double-thin-shell approach and TEC perturbation component to sound night-time mid-latitude E–F coupling

Fig. 4

2-D maps of input (a, b), IPP distribution (c, d), output (e, f) irregularities at E- and F-shell heights, a scatter of input and output total electron content perturbation (TECP) values (g) and a distribution of residuals (h) using GNSS signal rays at 17:30 JST, on 21 May 2010 (DOY 141). The yellow dashed line indicates a region, where reconstruction is of highest confidence level

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