Electron Acceleration Simulations (EASI): An open-source tool to simulate electron acceleration in shocks

dc.contributor.authorNyberg, Seve
dc.contributor.authorVuorinen, Laura
dc.contributor.authorAfanasiev, Alexandr
dc.contributor.authorAnnie John, Lidiya
dc.contributor.authorVainio, Rami
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id523444422
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/523444422
dc.date.accessioned2026-05-19T20:11:23Z
dc.description.abstract<p><em>Aims.</em> The aim of the this work is to investigate electron acceleration in shocks and present an easy-to-use simulation model that can be used to check resulting energetic particle populations from shock interactions.</p><p><em>Methods.</em> A new open-source model is presented in the work for investigation of electron acceleration and electron beam generation and for further research within the heliophysics community. The model is a one-dimensional Monte Carlo model with physical input parameters, in which particles obey a transport equation in a large-scale field with focusing caused by magnetic field gradients and in which the effects of a small-scale turbulent field on charged particles are described by pitch-angle scattering. The shock has a finite thickness and an adjustable mean free path profile. Particles are injected monoenergetically and with energies sampled from a Maxwellian distribution to investigate attained energies and beam generation.</p><p><em>Results.</em> The simulation results indicate that particles can be accelerated to energies of >100 keV from a 1 keV monoenergetic injection with plasma and shock parameters corresponding to coronal shock environments. An electron beam linked to radio observations of shock waves can also be generated with sufficiently high shock obliquities and, in particular, with a Maxwellian distribution of particle injection energies. Moreover, as the model performs computationally well and corresponds to expectations based on physics, it is an excellent tool for investigating energetic electrons and radio observations corresponding to the electron beams generated in shock waves.</p>
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.urihttps://www.utupub.fi/handle/11111/60903
dc.identifier.urlhttps://doi.org/10.1051/0004-6361/202557951
dc.identifier.urnURN:NBN:fi-fe2026051949737
dc.language.isoen
dc.okm.affiliatedauthorNyberg, Seve
dc.okm.affiliatedauthorVuorinen, Laura
dc.okm.affiliatedauthorAfanasiev, Alexandr
dc.okm.affiliatedauthorAnnie John, Lidiya
dc.okm.affiliatedauthorVainio, Rami
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.discipline114 Physical sciencesen_GB
dc.okm.discipline114 Fysiikkafi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherEDP Sciences
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberA67
dc.relation.doi10.1051/0004-6361/202557951
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume708
dc.titleElectron Acceleration Simulations (EASI): An open-source tool to simulate electron acceleration in shocks
dc.year.issued2026

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