The long period of 3He-rich solar energetic particles measured by Solar Orbiter 2020 November 17–23

dc.contributor.authorBucik R
dc.contributor.authorMason GM
dc.contributor.authorGomez-Herrero R
dc.contributor.authorLario D
dc.contributor.authorBalmaceda L
dc.contributor.authorNitta NV
dc.contributor.authorKrupar V
dc.contributor.authorDresing Nina
dc.contributor.authorHo GC
dc.contributor.authorAllen RC
dc.contributor.authorCarcaboso F
dc.contributor.authorRodriguez-Pacheco J
dc.contributor.authorSchuller F
dc.contributor.authorWarmuth A
dc.contributor.authorWimmer-Schweingruber RF
dc.contributor.authorvon Forstner JLF
dc.contributor.authorAndrews GB
dc.contributor.authorBerger L
dc.contributor.authorCernuda I
dc.contributor.authorLara FE
dc.contributor.authorLees WJ
dc.contributor.authorMartin C
dc.contributor.authorPacheco D
dc.contributor.authorPrieto M
dc.contributor.authorSanchez-Prieto S
dc.contributor.authorSchlemm CE
dc.contributor.authorSeifert H
dc.contributor.authorTyagi K
dc.contributor.authorMaksimovic M
dc.contributor.authorVecchio A
dc.contributor.authorKollhoff A
dc.contributor.authorKuhl P
dc.contributor.authorXu ZG
dc.contributor.authorEldrum S
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id68657645
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/68657645
dc.date.accessioned2022-10-28T12:27:27Z
dc.date.available2022-10-28T12:27:27Z
dc.description.abstractWe 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.
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid176534
dc.identifier.oldhandle10024/159628
dc.identifier.urihttps://www.utupub.fi/handle/11111/31989
dc.identifier.urlhttps://www.aanda.org/articles/aa/full_html/2021/12/aa41009-21/aa41009-21.html
dc.identifier.urnURN:NBN:fi-fe2022012710681
dc.language.isoen
dc.okm.affiliatedauthorGieseler, Nina
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeB1 Scientific Journal
dc.publisherEDP SCIENCES S A
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberARTN L11
dc.relation.doi10.1051/0004-6361/202141009
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume656
dc.source.identifierhttps://www.utupub.fi/handle/10024/159628
dc.titleThe long period of 3He-rich solar energetic particles measured by Solar Orbiter 2020 November 17–23
dc.year.issued2021

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