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...

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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

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