Heavy-ion acceleration and self-generated waves in coronal shocks

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dc.contributor.authorBattarbee M
dc.contributor.authorLaitinen T
dc.contributor.authorVainio R
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code2606702
dc.converis.publication-id2125978
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/2125978
dc.date.accessioned2022-10-28T14:19:44Z
dc.date.available2022-10-28T14:19:44Z
dc.description.abstract<p> Conclusions. We suggest that understanding the acceleration of minor ions at coronal shocks requires simulations which allow us to explore trapping dynamics and acceleration timescales in detail, including evolution of the turbulent trapping boundary. We conclude that steady-state models do not adequately describe the acceleration of heavy ions in coronal shocks.</p>
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid187625
dc.identifier.oldhandle10024/170719
dc.identifier.urihttps://www.utupub.fi/handle/11111/43134
dc.identifier.urnURN:NBN:fi-fe2021042714481
dc.language.isoen
dc.okm.affiliatedauthorBattarbee, Markus
dc.okm.discipline114 Physical sciencesen_GB
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline114 Fysiikkafi_FI
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherEDP SCIENCES S A
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberARTN A34
dc.relation.doi10.1051/0004-6361/201117507
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume535
dc.source.identifierhttps://www.utupub.fi/handle/10024/170719
dc.titleHeavy-ion acceleration and self-generated waves in coronal shocks
dc.year.issued2011

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