Fig. B.2.
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Similar to Fig. B.1 but now showing the PFSS magnetic field lines from PSP to the solar surface coloured red when the predicted magnetic field polarity does not match the in situ measurement. The grey scale shows Carrington maps of SDO/AIA 304Å emission. The fraction of hourly magnetic field polarity that matched the PFSS model is given in the upper-right corner for each encounter.
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