Wavefront error of PHI/HRT on Solar Orbiter at various heliocentric distances

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 15.

Same as Fig. 14 but for the noise measured in the LOS magnetic field maps of the RSW2 datasets. The noise is measured from Gaussian fits to the histograms of the B_los distribution as described in Liu et al. (2012).

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