Four Distinct Pathways to the Element Abundances in Solar Energetic Particles
Donald V. Reames

TL;DR
This paper identifies four distinct pathways that produce different element abundance patterns in solar energetic particles, based on their origin, acceleration, and transport mechanisms.
Contribution
It introduces a comprehensive classification of SEP populations based on recent abundance pattern evidence and their associated physical processes.
Findings
Four SEP populations with distinct abundance patterns identified
Different acceleration and reacceleration processes characterized
Element abundances linked to specific solar and CME conditions
Abstract
Based upon recent evidence from abundance patterns of chemical elements in solar energetic particles (SEPs), and, ironically, the belated inclusion of H and He, we can distinguish four basic SEP populations: (1) SEP1 - pure "impulsive" SEPs are produced by magnetic reconnection in solar jets showing steep power-law enhancements of 1<= Z <= 56 ions versus charge-to-mass ratio A/Q from a ~3 MK plasma. (2) SEP2 - ambient ions, mostly protons, plus SEP1 ions reaccelerated by the shock wave driven by the narrow coronal mass ejection (CME) from the same jet. (3) SEP3 - a "gradual" SEP event is produced when a moderately fast, wide CME-driven shock wave barely accelerates ambient protons while preferentially accelerating accumulated remnant SEP1 ions from an active region fed by multiple jets. (4) SEP4 - a gradual SEP event is produced when a very fast, wide CME-driven shock wave is completely…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
