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Doppler map of line Fe XIII 202.044 Å is obtained from synthetic spectral image using the magnetic boundary of Carrington Rotation 2082, as could be perceived from Earth after the line-of-sight integration of individual emission lines (from Szente et al., 2019). Blueshifts show regions where the solar wind is moving toward the observer, redshifts are present where plasma is moving away from the observer. The denser the plasma, the more dominant its effect is on the overall integrated Doppler shift of the observed line.
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