Intensity contrast of solar network and faculae close to the solar limb, observed from two vantage points

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 5.

Same as Fig. 4, but now showing facular contrast vs. μ. The data are displayed in six intervals of B_LOS/μ, and in bins of Δμ = 0.05. The third order fit here is done through the combined points, extended with the points derived from SO/PHI only data where μ > 0.4.

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