PROBA2/SWAP EUV images of the large-scale EUV corona up to 3 solar radii: Can we close the gap in coronal magnetic field structure between 1.3 and 2.5 solar radii? - De Groof, A. et al - Talk presented at Joint American Astronomical Society/American Geophysical Union Triennial Earth-Sun Summit, meeting #1, #409.01 on 2015-xx-xx - SIDCimport-1199
 
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