High dispersion solar spectrum. A code implementation for its analysis

A code is presented which allows first direct analysis of the Sacrament Peak Observatory's high resolution spectral atlas of the solar irradiance (from 380 to 700 nanometers) in the OAC's Microvax II system and also in the IBM 3031 of the University of Córdoba. The photometric data are spa...

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Detalles Bibliográficos
Autor principal: Villada, Mónica
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1987
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/137628
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-137628
record_format dspace
spelling I19-R120-10915-1376282024-10-16T18:45:51Z http://sedici.unlp.edu.ar/handle/10915/137628 High dispersion solar spectrum. A code implementation for its analysis Villada, Mónica 1987 2022-06-09T15:41:11Z es Astronomía Galaxias A code is presented which allows first direct analysis of the Sacrament Peak Observatory's high resolution spectral atlas of the solar irradiance (from 380 to 700 nanometers) in the OAC's Microvax II system and also in the IBM 3031 of the University of Córdoba. The photometric data are spaced 0.005 Å in the 3800-7000 Å region and calibration constants are provided which allow transformation to absolute values of intensities. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Villada, Mónica
High dispersion solar spectrum. A code implementation for its analysis
topic_facet Astronomía
Galaxias
description A code is presented which allows first direct analysis of the Sacrament Peak Observatory's high resolution spectral atlas of the solar irradiance (from 380 to 700 nanometers) in the OAC's Microvax II system and also in the IBM 3031 of the University of Córdoba. The photometric data are spaced 0.005 Å in the 3800-7000 Å region and calibration constants are provided which allow transformation to absolute values of intensities.
format Articulo
Comunicacion
author Villada, Mónica
author_facet Villada, Mónica
author_sort Villada, Mónica
title High dispersion solar spectrum. A code implementation for its analysis
title_short High dispersion solar spectrum. A code implementation for its analysis
title_full High dispersion solar spectrum. A code implementation for its analysis
title_fullStr High dispersion solar spectrum. A code implementation for its analysis
title_full_unstemmed High dispersion solar spectrum. A code implementation for its analysis
title_sort high dispersion solar spectrum. a code implementation for its analysis
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/137628
work_keys_str_mv AT villadamonica highdispersionsolarspectrumacodeimplementationforitsanalysis
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