Work

In-depth Analysis of the 2022 March 28 3He-rich Solar Energetic Particle Event

Year: 2025
Type: article
Abstract: On 2022 March 28, a solar eruption from active region AR 12975 produced a solar energetic particle (SEP) event observed by BepiColombo (BC; 0.57 au), STEREO-A (STA; 0.97 au), GOES (1.0 au), ACE (L1), and Wind (L1). The event was associated with an M4.0 soft X-ray flare peaking at 11:29 UTC, a Type III radio burst (0.1–16 MHz) at 11:24 UTC, a metric Type II radio burst (25–250 MHz) at 11:23 UTC, and a coronal mass ejection with a speed of 700 km s−1. BC and STA, magnetically aligned along the same Parker spiral and well connected to the flare site (footpoint separations of 19 . ° 8 and 16 . ° 5, respectively), detected a gradual SEP event with remarkable impulsive characteristics, including a high 3He/4He ratio (0.7 at 1 MeV), elevated Fe/O ratio (∼0.5 increasing with energy), a 3He spectrum harder than that of other ions, and particle dropouts at BC linked to intermittent magnetic connections. Near-Earth spacecraft (44 . ° 8 from the flare site) observed abundance ratios closer to coronal values, and more uniform proton/heavy-ion spectra. Our findings suggest both the contribution of particles accelerated by a quasi-parallel shock and a direct contribution from flare suprathermals, accelerated during postflare ongoing reconnection, at well connected spacecraft.
Language: English
Open Access status: gold
Estimated APC paid: $4,499
OpenAlex ID: W4411834171
FWCI:
Cites: 76
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Related to: 10