Suprathermal Ions

Suprathermal ions have more energy than regular solar wind particles but less than those in solar storms. These particles seem to come from both continuous processes (like turbulence or magnetic reconnection) and past energetic events (like solar flares or shocks). Their composition and energy patterns vary with the solar cycle, suggesting that during quiet periods, they are leftover from previous events. Their consistent power-law energy distribution supports the idea that multiple overlapping processes contribute to their formation.

Figure showing suprathermal ion spectral index
A stackd histogram of the suprathermal ion spectral index (). The different colors indicate different elements. The white circle and line indicates the average . This spectral index is invariant across solar activity. From Alterman et al. (2024), The Astrophysical Journal Letters.