Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis

Abstract: Six existing models and one proposed approach for estimating global solar radiation were tested in Buenos Aires using commonly measured meteorological data as temperature and sunshine hours covering the years 2010-2013. Statistical predictors as mean bias error, root mean square, mean perc...

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Autores principales: Lakkis, Susan Gabriela, Lavorato, Mario, Canziani, Pablo O.
Otros Autores: Universidad Católica Argentina (Buenos Aires). Facultad de Ciencias Agrarias
Formato: Artículo
Lenguaje:Inglés
Publicado: 2019
Materias:
Acceso en línea:https://repositorio.uca.edu.ar/handle/123456789/5434
Aporte de:
id I33-R139-123456789-5434
record_format dspace
spelling I33-R139-123456789-54342024-03-07T12:26:13Z Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis Lakkis, Susan Gabriela Lavorato, Mario Canziani, Pablo O. Universidad Católica Argentina (Buenos Aires). Facultad de Ciencias Agrarias Consejo Nacional de Investigaciones Científicas y Técnicas (Argentina) RADIACION SOLAR METEOROLOGIA ESTRADISTICAS Abstract: Six existing models and one proposed approach for estimating global solar radiation were tested in Buenos Aires using commonly measured meteorological data as temperature and sunshine hours covering the years 2010-2013. Statistical predictors as mean bias error, root mean square, mean percentage error, slope and regression coefficients were used as validation criteria. The variability explained (R2), slope and MPE indicated that the higher precision could be excepted when sunshine hours are used as predictor. The new proposed approach explained almost 99% of the RG variability with deviation of less than ± 0.1 MJm-2day-1 and with the MPE smallest value below 1 %. The well known Ångström-Prescott methods, first and third order, was also found to perform for the measured data with high accuracy (R2=0.97-0.99) but with slightly higher MBE values (0.17-0.18 MJm-2day-1). The results pointed out that the third order Ångström type correlation did not improve the estimation accuracy of solar radiation given the highest range of deviation and mean percentage error obtained. Where the sunshine hours were not available, the formulae including temperature data might be considered as an alternative although the methods displayed larger deviation and tended to overestimate the solar radiation behavior 2019-06-06T00:48:15Z 2019-06-06T00:48:15Z 2014 Artículo Lakkis, S. G., Lavorato, M. y P. O. Canziani. 2014. Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis [en línea]. Journal of advances in physics 5(1). Disponible en: https://repositorio.uca.edu.ar/handle/123456789/5434 2347-3487 https://repositorio.uca.edu.ar/handle/123456789/5434 eng Acceso Abierto https://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf BUENOS AIRES ARGENTINA Journal of Advances in Physics, Vol. 5, Nro. 1, 2014 ISSN 2347-3487
institution Universidad Católica Argentina
institution_str I-33
repository_str R-139
collection Repositorio Institucional de la Universidad Católica Argentina (UCA)
language Inglés
topic RADIACION SOLAR
METEOROLOGIA
ESTRADISTICAS
spellingShingle RADIACION SOLAR
METEOROLOGIA
ESTRADISTICAS
Lakkis, Susan Gabriela
Lavorato, Mario
Canziani, Pablo O.
Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
topic_facet RADIACION SOLAR
METEOROLOGIA
ESTRADISTICAS
description Abstract: Six existing models and one proposed approach for estimating global solar radiation were tested in Buenos Aires using commonly measured meteorological data as temperature and sunshine hours covering the years 2010-2013. Statistical predictors as mean bias error, root mean square, mean percentage error, slope and regression coefficients were used as validation criteria. The variability explained (R2), slope and MPE indicated that the higher precision could be excepted when sunshine hours are used as predictor. The new proposed approach explained almost 99% of the RG variability with deviation of less than ± 0.1 MJm-2day-1 and with the MPE smallest value below 1 %. The well known Ångström-Prescott methods, first and third order, was also found to perform for the measured data with high accuracy (R2=0.97-0.99) but with slightly higher MBE values (0.17-0.18 MJm-2day-1). The results pointed out that the third order Ångström type correlation did not improve the estimation accuracy of solar radiation given the highest range of deviation and mean percentage error obtained. Where the sunshine hours were not available, the formulae including temperature data might be considered as an alternative although the methods displayed larger deviation and tended to overestimate the solar radiation behavior
author2 Universidad Católica Argentina (Buenos Aires). Facultad de Ciencias Agrarias
author_facet Universidad Católica Argentina (Buenos Aires). Facultad de Ciencias Agrarias
Lakkis, Susan Gabriela
Lavorato, Mario
Canziani, Pablo O.
format Artículo
author Lakkis, Susan Gabriela
Lavorato, Mario
Canziani, Pablo O.
author_sort Lakkis, Susan Gabriela
title Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
title_short Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
title_full Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
title_fullStr Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
title_full_unstemmed Estimation of monthly global solar radiation in Buenos Aires : preliminary analysis
title_sort estimation of monthly global solar radiation in buenos aires : preliminary analysis
publishDate 2019
url https://repositorio.uca.edu.ar/handle/123456789/5434
work_keys_str_mv AT lakkissusangabriela estimationofmonthlyglobalsolarradiationinbuenosairespreliminaryanalysis
AT lavoratomario estimationofmonthlyglobalsolarradiationinbuenosairespreliminaryanalysis
AT canzianipabloo estimationofmonthlyglobalsolarradiationinbuenosairespreliminaryanalysis
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