Improving the Ni i atomic model for solar and stellar atmospheric models

Neutral nickel (Ni I) is abundant in the solar atmosphere and is one of the important elements that contribute to the emission and absorption of radiation in the spectral range between 1900 and 3900 Å. Previously, the Solar Radiation Physical Modeling (SRPM) models of the solar atmosphere only consi...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Vieytes, M.C., Fontenla, J.M.
Formato: JOUR
Materias:
line: formation
radiative transfer
Sun: atmosphere
Sun: UV radiation
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v769_n2_p_Vieytes
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_0004637X_v769_n2_p_Vieytes
record_format dspace
spelling todo:paper_0004637X_v769_n2_p_Vieytes2023-10-03T14:02:33Z Improving the Ni i atomic model for solar and stellar atmospheric models Vieytes, M.C. Fontenla, J.M. line: formation radiative transfer Sun: atmosphere Sun: UV radiation Neutral nickel (Ni I) is abundant in the solar atmosphere and is one of the important elements that contribute to the emission and absorption of radiation in the spectral range between 1900 and 3900 Å. Previously, the Solar Radiation Physical Modeling (SRPM) models of the solar atmosphere only considered a few levels of this species. Here, we improve the Ni I atomic model by taking into account 61 levels and 490 spectral lines. We compute the populations of these levels in full NLTE using the SRPM code and compare the resulting emerging spectrum with observations. The present atomic model significantly improves the calculation of the solar spectral irradiance at near-UV wavelengths, which is important for Earth atmospheric studies, and particularly for ozone chemistry. © 2013. The American Astronomical Society. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v769_n2_p_Vieytes
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic line: formation
radiative transfer
Sun: atmosphere
Sun: UV radiation
spellingShingle line: formation
radiative transfer
Sun: atmosphere
Sun: UV radiation
Vieytes, M.C.
Fontenla, J.M.
Improving the Ni i atomic model for solar and stellar atmospheric models
topic_facet line: formation
radiative transfer
Sun: atmosphere
Sun: UV radiation
description Neutral nickel (Ni I) is abundant in the solar atmosphere and is one of the important elements that contribute to the emission and absorption of radiation in the spectral range between 1900 and 3900 Å. Previously, the Solar Radiation Physical Modeling (SRPM) models of the solar atmosphere only considered a few levels of this species. Here, we improve the Ni I atomic model by taking into account 61 levels and 490 spectral lines. We compute the populations of these levels in full NLTE using the SRPM code and compare the resulting emerging spectrum with observations. The present atomic model significantly improves the calculation of the solar spectral irradiance at near-UV wavelengths, which is important for Earth atmospheric studies, and particularly for ozone chemistry. © 2013. The American Astronomical Society. All rights reserved.
format JOUR
author Vieytes, M.C.
Fontenla, J.M.
author_facet Vieytes, M.C.
Fontenla, J.M.
author_sort Vieytes, M.C.
title Improving the Ni i atomic model for solar and stellar atmospheric models
title_short Improving the Ni i atomic model for solar and stellar atmospheric models
title_full Improving the Ni i atomic model for solar and stellar atmospheric models
title_fullStr Improving the Ni i atomic model for solar and stellar atmospheric models
title_full_unstemmed Improving the Ni i atomic model for solar and stellar atmospheric models
title_sort improving the ni i atomic model for solar and stellar atmospheric models
url http://hdl.handle.net/20.500.12110/paper_0004637X_v769_n2_p_Vieytes
work_keys_str_mv AT vieytesmc improvingtheniiatomicmodelforsolarandstellaratmosphericmodels
AT fontenlajm improvingtheniiatomicmodelforsolarandstellaratmosphericmodels
_version_ 1807317817624625152

Ejemplares similares