NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension

Detalhes bibliográficos
Autor(a) principal: de Avillez, Miguel
Data de Publicação: 2010
Outros Autores: Breitschwerdt, Dieter
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10174/5641
https://doi.org/10.1017/S1743921310010318
Resumo: High-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.
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spelling NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff DimensionHigh-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.Cambridge University Press/International Astronomical Union2012-11-15T14:22:01Z2012-11-152010-11-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://hdl.handle.net/10174/5641http://hdl.handle.net/10174/5641https://doi.org/10.1017/S1743921310010318eng468-46915mavillez@galaxy.lca.uevora.ptbreitschwerdt@astro.physik.tu-berlin.deHighlights of Astronomy343de Avillez, MiguelBreitschwerdt, Dieterinfo: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:RCAAP2024-01-03T18:44:40Zoai:dspace.uevora.pt:10174/5641Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T01:00:40.791621Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
title NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
spellingShingle NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
de Avillez, Miguel
title_short NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
title_full NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
title_fullStr NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
title_full_unstemmed NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
title_sort NEI Modelling of the ISM - Turbulent Dissipation and Hausdorff Dimension
author de Avillez, Miguel
author_facet de Avillez, Miguel
Breitschwerdt, Dieter
author_role author
author2 Breitschwerdt, Dieter
author2_role author
dc.contributor.author.fl_str_mv de Avillez, Miguel
Breitschwerdt, Dieter
description High-resolution non-ideal magnetohydrodynamical simulations of the turbulent magnetized ISM, powered by supernovae types Ia and II at Galactic rate, including self-gravity and non-equilibriuim ionization (NEI), taking into account the time evolution of the ionization structure of H, He, C, N, O, Ne, Mg, Si, S and Fe, were carried out. These runs cover a wide range (from kpc to sub-parsec) of scales, providing resolution independent information on the injection scale, extended self-similarity and the fractal dmension of the most dissipative structures.
publishDate 2010
dc.date.none.fl_str_mv 2010-11-01T00:00:00Z
2012-11-15T14:22:01Z
2012-11-15
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/10174/5641
http://hdl.handle.net/10174/5641
https://doi.org/10.1017/S1743921310010318
url http://hdl.handle.net/10174/5641
https://doi.org/10.1017/S1743921310010318
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 468-469
15
mavillez@galaxy.lca.uevora.pt
breitschwerdt@astro.physik.tu-berlin.de
Highlights of Astronomy
343
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Cambridge University Press/International Astronomical Union
publisher.none.fl_str_mv Cambridge University Press/International Astronomical Union
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
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reponame_str Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
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repository.name.fl_str_mv Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação
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