Reconstructing solar magnetic fields from historical observations - X. Effect of magnetic field inclination and boundary structure on AIA 1600 Å emission

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Fig. 5.

Peak median AIA 1600 intensities from Figs. 4c and 4d as a function of local inclination. Error bars correspond to twice the bootstrap standard error. The solid lines show the best cosine fits to peak intensities. Dashed lines show 95% confidence bounds of the cosine fit.

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