Monte Carlo simulations of nuclear de-excitation gamma-ray line spectra from solar flares

dc.contributor.authorSzpigel S.
dc.contributor.authorThereza R.M.
dc.contributor.authorde Castro C.G.G.
dc.contributor.authorMacKinnon A.L.
dc.contributor.authorde Aguiar Simoes P.J.
dc.date.accessioned2024-03-12T19:16:55Z
dc.date.available2024-03-12T19:16:55Z
dc.date.issued2022
dc.description.abstract© 2022 Institute of Physics Publishing. All rights reserved.Recently, we have demonstrated that the Monte Carlo package FLUKA can be used as an effective tool for simulating nuclear processes which occur in solar flares and that it is capable to provide a self-consistent treatment of all typical components of the γ-ray spectra observed in those events. In this work, we have employed a new simulation strategy that allows to improve statistics and resolution in energy of the generated γ-ray spectra. Using this new strategy, we have calculated spectra of γ-ray nuclear de-excitation lines produced by solar flare primary accelerated ions with typical power-law energy distributions.
dc.description.issuenumber1
dc.description.volume2340
dc.identifier.doi10.1088/1742-6596/2340/1/012031
dc.identifier.issn1742-6596
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/34469
dc.relation.ispartofJournal of Physics: Conference Series
dc.rightsAcesso Aberto
dc.titleMonte Carlo simulations of nuclear de-excitation gamma-ray line spectra from solar flares
dc.typeArtigo de evento
local.scopus.citations0
local.scopus.eid2-s2.0-85140231785
local.scopus.subjectDe-excitations
local.scopus.subjectEffective tool
local.scopus.subjectGamma-ray line
local.scopus.subjectLine spectra
local.scopus.subjectMonte Carlo's simulation
local.scopus.subjectNuclear process
local.scopus.subjectSelf-consistent treatment
local.scopus.subjectSimulation strategies
local.scopus.subjectSolar flare
local.scopus.subjectSpectra's
local.scopus.updated2024-06-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85140231785&origin=inward
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