Assessment of the near-Sun magnetic field of the 10 March 2022 coronal mass ejection observed by Solar Orbiter

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 10.

CME magnetic field variation with distance. Blue points with error bars depict the maximum magnetic field B₀. The near-Sun field is estimated, while the fields at 0.43 AU (Solar Orbiter) and 0.99 AU (WIND) rely on in situ measurements. The 0.99 AU measurements have minimal error (on the order pT), and the red line represents the least-squares best fit.

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