The multi-spacecraft high-energy solar particle event of 28 October 2021

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 8.

Spectra and relative abundance over the entire event. Top: Differential fluence spectra for major species. The dashed lines connect gaps in instrumental energy coverage and are only to guide the eye. Bottom: Relative abundance of ions measured over the energy range 320–450 keV nucleon⁻¹ from SOLO/SIS, ACE/ULEIS, and the survey of Desai et al. (2006).

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