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Fig. 7.


Plots of α(θ) = Jr(R0, θ)/cρGJ in the parallel (panel a) and anti-parallel (panel b) configurations, for the top (top panel) and bottom (bottom panel) pulsars. The stellar distance is fixed at a = 3 RLC. The dashed lines mark the locations of θpc and π − θpc (see Eq. (12)). The grey-shaded zones indicate the inward pole regions of emission, and the color-shaded zones mark the outward pole emission.

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