The long period of 3He-rich solar energetic particles measured by Solar Orbiter 2020 November 17–23
Wimmer-Schweingruber RF; Tyagi K; Maksimovic M; Schlemm CE; Seifert H; Kollhoff A; Sanchez-Prieto S; Andrews GB; Pacheco D; Mason GM; Bucik R; Ho GC; Carcaboso F; Vecchio A; Prieto M; Nitta NV; Gomez-Herrero R; von Forstner JLF; Lees WJ; Berger L; Allen RC; Lara FE; Cernuda I; Dresing Nina; Krupar V; Kuhl P; Schuller F; Eldrum S; Warmuth A; Balmaceda L; Martin C; Xu ZG; Rodriguez-Pacheco J; Lario D
The long period of 3He-rich solar energetic particles measured by Solar Orbiter 2020 November 17–23
Wimmer-Schweingruber RF
Tyagi K
Maksimovic M
Schlemm CE
Seifert H
Kollhoff A
Sanchez-Prieto S
Andrews GB
Pacheco D
Mason GM
Bucik R
Ho GC
Carcaboso F
Vecchio A
Prieto M
Nitta NV
Gomez-Herrero R
von Forstner JLF
Lees WJ
Berger L
Allen RC
Lara FE
Cernuda I
Dresing Nina
Krupar V
Kuhl P
Schuller F
Eldrum S
Warmuth A
Balmaceda L
Martin C
Xu ZG
Rodriguez-Pacheco J
Lario D
EDP SCIENCES S A
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2022012710681
https://urn.fi/URN:NBN:fi-fe2022012710681
Tiivistelmä
We report observations of a relatively long period of He-3-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injections. The high-resolution STEREO-A imaging observations reveal that the injections coincide with extreme ultraviolet jets and brightenings near the east limb, not far from the nominal magnetic connection of Solar Orbiter. The jets originated in two adjacent, large, and complex active regions, as observed by the Solar Dynamics Observatory when the regions rotated into the Earth's view. It appears that the sustained ion injections were related to the complex configuration of the sunspot group and the long period of He-3-rich SEPs to the longitudinal extent covered by the group during the analyzed time period.
Kokoelmat
- Rinnakkaistallenteet [19207]