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Fig. 12.

Fig. 12. Refer to the following caption and surrounding text.

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Second-order two- and three-point structure functions for the polarised intensity of the northern region. The blue and grey dashed vertical lines indicate the telescope’s beam size, lb, and coherence length, ls, respectively. The black and blue dashed horizontal lines mark 2σ2 and 2 σ s 2 Mathematical equation: $ \sigma_{s}^{2} $, corresponding to the variance for initial polarised intensity and small-scale fluctuations, respectively.

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