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Comparing extrapolations of the coronal magnetic field structure at 2.5<i>R</i><sub>โ</sub>with multi-viewpoint coronagraphic observations
The magnetic field shapes the structure of the solar corona but we still know little about the interrelationships between the coronal magnetic field configurations and the resulting quasi-stationary structures observed in coronagraphic images (as streamers, plumes, coronal holes). One way to obtain information on the large-scale structure of the coronal โฆ