Experimental estimation of the luminosity of the Sun

We determine the solar constant experimentally using two independent techniques that allow us to study the dependence of the solar irradiation on the zenith angle and the characteristics of the light extinction in the atmosphere. Our result for the solar luminosity agrees within 7% of the accepted v...

Descripción completa

Detalles Bibliográficos
Autor principal: Pellizza Gonzalez, Leonardo Javier
Publicado: 2006
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00029505_v74_n8_p728_Gil
http://hdl.handle.net/20.500.12110/paper_00029505_v74_n8_p728_Gil
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00029505_v74_n8_p728_Gil
record_format dspace
spelling paper:paper_00029505_v74_n8_p728_Gil2023-06-08T14:23:13Z Experimental estimation of the luminosity of the Sun Pellizza Gonzalez, Leonardo Javier We determine the solar constant experimentally using two independent techniques that allow us to study the dependence of the solar irradiation on the zenith angle and the characteristics of the light extinction in the atmosphere. Our result for the solar luminosity agrees within 7% of the accepted value. This value can be used to estimate the luminosity or power radiated by the Sun. The experiment is inexpensive and conceptually easy to perform and understand. © 2006 American Association of Physics Teachers. Fil:Pellizza, L.J. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2006 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00029505_v74_n8_p728_Gil http://hdl.handle.net/20.500.12110/paper_00029505_v74_n8_p728_Gil
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description We determine the solar constant experimentally using two independent techniques that allow us to study the dependence of the solar irradiation on the zenith angle and the characteristics of the light extinction in the atmosphere. Our result for the solar luminosity agrees within 7% of the accepted value. This value can be used to estimate the luminosity or power radiated by the Sun. The experiment is inexpensive and conceptually easy to perform and understand. © 2006 American Association of Physics Teachers.
author Pellizza Gonzalez, Leonardo Javier
spellingShingle Pellizza Gonzalez, Leonardo Javier
Experimental estimation of the luminosity of the Sun
author_facet Pellizza Gonzalez, Leonardo Javier
author_sort Pellizza Gonzalez, Leonardo Javier
title Experimental estimation of the luminosity of the Sun
title_short Experimental estimation of the luminosity of the Sun
title_full Experimental estimation of the luminosity of the Sun
title_fullStr Experimental estimation of the luminosity of the Sun
title_full_unstemmed Experimental estimation of the luminosity of the Sun
title_sort experimental estimation of the luminosity of the sun
publishDate 2006
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00029505_v74_n8_p728_Gil
http://hdl.handle.net/20.500.12110/paper_00029505_v74_n8_p728_Gil
work_keys_str_mv AT pellizzagonzalezleonardojavier experimentalestimationoftheluminosityofthesun
_version_ 1768541587008126976

Ejemplares similares