Backstreaming ions at a high Mach number interplanetary shock - Solar Orbiter measurements during the nominal mission phase

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 3.

Overview of the IP shock observed by Solar Orbiter on 30 October 2021. Panels a–k from top to bottom represent |B|, B_rtn, E_rtn, n_i, e, T_i, V_rtn, EPD ion energy, SWA-PAS differential energy flux, B wavelet spectra, E wavelet spectra, and the ellipticity of B. The shock crossing occurs around 22:02 UTC and is marked by the sudden change in all the plotted quantities.

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