Solar Activities Associated with 3He-rich Solar Energetic Particle Events Observed by Solar Orbiter

Impulsive solar energetic particle (SEP) events are distinguished from shock-accelerated gradual SEP events especially in terms of their abundance enriched in ³He and heavy ions. Historically, ³He-rich  have been known to be accompanied by type III radio bursts and energetic electrons. For more than 15 years in the past it has often been proclaimed that coronal jets are responsible for ³He-rich SEP events. We revisit the link of ³He-rich SEP events with coronal jets in a series of ³He-rich SEP events that was observed by Solar Orbiter in May 2021 at a radial distance of 0.95 AU. An isolated active region AR 12824 was likely the ultimate source of these SEP events.  The period of the enhanced flux of ³He was also a period of frequent type III bursts in the  decametric-hectometric range, confirming their close relationship. As in past studies, we try to find the solar activities possibly responsible for ³He-rich SEP events, using the type III bursts close to the particle injection times estimated from the velocity dispersion. But this exercise is not as straightforward as in many of the past studies since the region produced many more type III bursts and jet-like eruptions than the SEP injections.  We may generalize the solar activities for the ³He-rich SEP events in question as coronal jets, but their appearances do not necessarily conform to classic jets that consist of a footpoint and a spire. Conversely, such jets often did not accompany type III bursts. The areas that produced jet-like eruptions changed within the active region from the first to the second set of ³He-rich SEP events, which may be related to the extended coronal mass ejection that launched stealthily, involving both the leading and trailing polarity areas of AR 12824.