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. A.1.

Scattered blue data points show in situ measurements of B_SolO over time. The red curve represents the quadratic fit approximating the data trends. Extrapolated linear fits of B_SolO nT and their intersection point (magenta dot) suggest potential B_0SolO at 0.43 AU.

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