Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
Texto Completo: | http://hdl.handle.net/10362/90034 |
Resumo: | Deutsche Forschungsgemeinschaft (DFG) Project No. 266229290. |
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Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
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Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channelsatomic dataatomic processesline: formationmethods: laboratory: atomicplasmasX-rays: generalAstronomy and AstrophysicsSpace and Planetary ScienceDeutsche Forschungsgemeinschaft (DFG) Project No. 266229290.We determined relative X-ray photon emission cross sections in Fe xvii ions that were mono-energetically excited in an electron beam ion trap. Line formation for the 3s (3s-2p) and 3d (3d-2p) transitions of interest proceeds through dielectronic recombination (DR), direct electron-impact excitation (DE), resonant excitation (RE), and radiative cascades. By reducing the electron-energy spread to a sixth of that of previous works and increasing counting statistics by three orders of magnitude, we account for hitherto unresolved contributions from DR and the little-studied RE process to the 3d transitions, and also for cascade population of the 3s line manifold through forbidden states. We found good agreement with state-of-the-art many-body perturbation theory (MBPT) and the distorted-wave (DW) method for the 3s transition, while in the 3d transitions known discrepancies were confirmed. Our results show that DW calculations overestimate the 3d line emission due to DE by ∼20%. Inclusion of electron-electron correlation effects through the MBPT method in the DE cross-section calculations reduces this disagreement by ∼11%. The remaining ∼9% in 3d and ∼11% in 3s/3d discrepancies are consistent with those found in previous laboratory measurements, solar, and astrophysical observations. Meanwhile, spectral models of opacity, temperature, and turbulence velocity should be adjusted to these experimental cross sections to optimize the accuracy of plasma diagnostics based on these bright soft X-ray lines of Fe xvii.LIBPhys-UNLDF – Departamento de FísicaRUNShah, ChintanLópez-Urrutia, José R.CrespoGu, Ming FengPfeifer, ThomasMarques, JoséGrilo, FilipeSantos, José PauloAmaro, Pedro2019-12-17T23:30:53Z2019-08-202019-08-20T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10362/90034eng0004-637XPURE: 15239925https://doi.org/10.3847/1538-4357/ab2896info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-07-10T15:52:07ZPortal AgregadorONG |
dc.title.none.fl_str_mv |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
title |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
spellingShingle |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels Shah, Chintan atomic data atomic processes line: formation methods: laboratory: atomic plasmas X-rays: general Astronomy and Astrophysics Space and Planetary Science |
title_short |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
title_full |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
title_fullStr |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
title_full_unstemmed |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
title_sort |
Revisiting the Fe xvii Line Emission Problem: Laboratory Measurements of the 3s-2p and 3d-2p Line-formation Channels |
author |
Shah, Chintan |
author_facet |
Shah, Chintan López-Urrutia, José R.Crespo Gu, Ming Feng Pfeifer, Thomas Marques, José Grilo, Filipe Santos, José Paulo Amaro, Pedro |
author_role |
author |
author2 |
López-Urrutia, José R.Crespo Gu, Ming Feng Pfeifer, Thomas Marques, José Grilo, Filipe Santos, José Paulo Amaro, Pedro |
author2_role |
author author author author author author author |
dc.contributor.none.fl_str_mv |
LIBPhys-UNL DF – Departamento de Física RUN |
dc.contributor.author.fl_str_mv |
Shah, Chintan López-Urrutia, José R.Crespo Gu, Ming Feng Pfeifer, Thomas Marques, José Grilo, Filipe Santos, José Paulo Amaro, Pedro |
dc.subject.por.fl_str_mv |
atomic data atomic processes line: formation methods: laboratory: atomic plasmas X-rays: general Astronomy and Astrophysics Space and Planetary Science |
topic |
atomic data atomic processes line: formation methods: laboratory: atomic plasmas X-rays: general Astronomy and Astrophysics Space and Planetary Science |
description |
Deutsche Forschungsgemeinschaft (DFG) Project No. 266229290. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-12-17T23:30:53Z 2019-08-20 2019-08-20T00:00:00Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10362/90034 |
url |
http://hdl.handle.net/10362/90034 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
0004-637X PURE: 15239925 https://doi.org/10.3847/1538-4357/ab2896 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação instacron:RCAAP |
instname_str |
Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
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Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
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1777302999899570176 |