Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications

The spectral distribution of the solar irradiance incident on photovoltaic (PV) modules is a key variable controlling their power production. It is required to properly simulate the production and performance of PV plants based on technologies with different spectral characteristics. Spectroradiomet...

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Main Authors: Gabriel López, Christian A. Gueymard, Jesús Polo, Joaquín Alonso-Montesinos, Aitor Marzo, Nuria Martín-Chivelet, Pablo Ferrada, Martha Isabel Escalona-Llaguno, Francisco Javier Batlles
Format: Article
Language:English
Published: MDPI AG 2023-03-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/15/6/1675
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author Gabriel López
Christian A. Gueymard
Jesús Polo
Joaquín Alonso-Montesinos
Aitor Marzo
Nuria Martín-Chivelet
Pablo Ferrada
Martha Isabel Escalona-Llaguno
Francisco Javier Batlles
author_facet Gabriel López
Christian A. Gueymard
Jesús Polo
Joaquín Alonso-Montesinos
Aitor Marzo
Nuria Martín-Chivelet
Pablo Ferrada
Martha Isabel Escalona-Llaguno
Francisco Javier Batlles
author_sort Gabriel López
collection DOAJ
description The spectral distribution of the solar irradiance incident on photovoltaic (PV) modules is a key variable controlling their power production. It is required to properly simulate the production and performance of PV plants based on technologies with different spectral characteristics. Spectroradiometers can only sense the solar spectrum within a wavelength range that is usually too short compared to the actual spectral response of some PV technologies. In this work, a new methodology based on the Simple Model of the Atmospheric Radiative Transfer of Sunshine (SMARTS) spectral code is proposed to extend the spectral range of measured direct irradiance spectra and to increase the spectral resolution of such experimental measurements. Satisfactory results were obtained for both clear and hazy sky conditions at a radiometric station in southern Spain. This approach constitutes the starting point of a general methodology to obtain the instantaneous spectral irradiance incident on the plane of array of PV modules and its temporal variations, while evaluating the magnitude and variability of the abundance of atmospheric constituents with the most impact on surface irradiance, most particularly aerosols and water vapor.
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spelling doaj.art-c07a0a1d3a234409998f6de34df472562023-11-17T13:40:24ZengMDPI AGRemote Sensing2072-42922023-03-01156167510.3390/rs15061675Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV ApplicationsGabriel López0Christian A. Gueymard1Jesús Polo2Joaquín Alonso-Montesinos3Aitor Marzo4Nuria Martín-Chivelet5Pablo Ferrada6Martha Isabel Escalona-Llaguno7Francisco Javier Batlles8Departamento Ingeniería Eléctrica y Térmica, de Diseño y Proyectos, Escuela Técnica Superior de Ingeniería, Universidad de Huelva, 21007 Huelva, SpainSolar Consulting Services, Colebrook, NH 03576, USAPhotovoltaic Solar Energy Unit (CIEMAT), 28040 Madrid, SpainDepartamento Química y Física, Universidad de Almería, 04120 Almería, SpainDepartamento Óptica, Universidad de Granada, 18071 Granada, SpainPhotovoltaic Solar Energy Unit (CIEMAT), 28040 Madrid, SpainCentro de Desarrollo Energético Antofagasta (CDEA), Universidad de Antofagasta, Antofagasta 1240000, ChileUniversidad Autónoma de Zacatecas, Zacatecas 98000, MexicoDepartamento Química y Física, Universidad de Almería, 04120 Almería, SpainThe spectral distribution of the solar irradiance incident on photovoltaic (PV) modules is a key variable controlling their power production. It is required to properly simulate the production and performance of PV plants based on technologies with different spectral characteristics. Spectroradiometers can only sense the solar spectrum within a wavelength range that is usually too short compared to the actual spectral response of some PV technologies. In this work, a new methodology based on the Simple Model of the Atmospheric Radiative Transfer of Sunshine (SMARTS) spectral code is proposed to extend the spectral range of measured direct irradiance spectra and to increase the spectral resolution of such experimental measurements. Satisfactory results were obtained for both clear and hazy sky conditions at a radiometric station in southern Spain. This approach constitutes the starting point of a general methodology to obtain the instantaneous spectral irradiance incident on the plane of array of PV modules and its temporal variations, while evaluating the magnitude and variability of the abundance of atmospheric constituents with the most impact on surface irradiance, most particularly aerosols and water vapor.https://www.mdpi.com/2072-4292/15/6/1675solar spectral irradianceSMARTSPVatmospheric constituentssoiling
spellingShingle Gabriel López
Christian A. Gueymard
Jesús Polo
Joaquín Alonso-Montesinos
Aitor Marzo
Nuria Martín-Chivelet
Pablo Ferrada
Martha Isabel Escalona-Llaguno
Francisco Javier Batlles
Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
Remote Sensing
solar spectral irradiance
SMARTS
PV
atmospheric constituents
soiling
title Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
title_full Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
title_fullStr Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
title_full_unstemmed Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
title_short Increasing the Resolution and Spectral Range of Measured Direct Irradiance Spectra for PV Applications
title_sort increasing the resolution and spectral range of measured direct irradiance spectra for pv applications
topic solar spectral irradiance
SMARTS
PV
atmospheric constituents
soiling
url https://www.mdpi.com/2072-4292/15/6/1675
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