Fig. 8
First-and second-order ionospheric effects quantified by variation of differential TEC and differential Faraday rotation between the LOFAR core and all remote stations. Each panel is a separate observation towards 3C380. The gaps between observations are: 21, 21, 21, 21, 72, 21, 21, and 44 hr. Stations are colour-coded in alphabetical order. The similarity between the top and bottom panels is due to the TEC dependency of Faraday rotation.
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