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. 4.

Wind L1 in situ observations (from top to bottom): a) magnetic-field components in the GSE system with the magnitude of the magnetic field, b) proton temperature, c) proton density, d) solar wind bulk velocity, and e) proton plasma β. The vertical orange dashed line marks the shock’s arrival, and the two black vertical dashed lines represent ICME start and end times.

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