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Fig. 4

image

Example of determining σw and pw by removing the π-component in the intensity profile (Stokes I; top left panel) in a pixel in which the magnetic field is aligned with the observer line of sight. Black lines represent the observed Stokes profiles Iobs. Red lines show the wide-angle contribution (i.e., scattered light) from the surrounding penumbra and quiet Sun, . Blue lines represent the observed Stokes profiles after removing 20% of the wide-angle contribution. See text for details.

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