Abstract

Knowledge of the solar radiation available on the earth’s surface is essential for the development of solar energy devices and for estimating of their performance efficiencies. For this purpose it is helpful to study the attenuation of direct normal irradiance by the atmosphere, in terms of fundamental quantities, including optical thickness, relative optical air mass, water vapor content, and aerosol amount. In the present article, we will not deal with cloudy atmospheres because of their great variability in space and time, but will focus our attention on atmospheres characterized by the complete absence of condensed water. The objectives of this article are to report data on aerosol optical depth and atmospheric turbidity coefficients for a desert climate, and to compare them with those of a temperate climate. Aerosol optical depth, the Linke turbidity factor, TL, and ngström turbidity coefficients, _, are calculated from measurements of broadband filters at Helwan, Egypt, which has a desert climate. A linear regression model is to be determined between the Linke factor and the ngström turbidity coefficient. This relation is compared with similar relations reported for a temperate climate [Prague, Czech Republic]. This comparison is made to determine whether a universal relation exists between these two important coefficients, or whether the relation is location dependent.

Highlights

  • The increase in terrestrial applications of solar radiant energy has given impetus to the study of solar energy availability in many areas of the world

  • When passing through the earth’s atmosphere, extraterrestrial solar radiation is subjected to attenuation due to scattering by the air molecules and aerosols, and due to absorption by various atmospheric components, mainly ozone, water vapor, oxygen and carbon dioxide

  • Regarding the global solar radiation data for Helwan and Cairo, it is found that the Helwan annual mean value was 5.48 kWh/m2/day, which is higher than the Cairo value, which was 5.03 kWh/m2/day

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Summary

Introduction

The increase in terrestrial applications of solar radiant energy has given impetus to the study of solar energy availability in many areas of the world. When passing through the earth’s atmosphere, extraterrestrial solar radiation is subjected to attenuation due to scattering by the air molecules and aerosols, and due to absorption by various atmospheric components, mainly ozone, water vapor, oxygen and carbon dioxide. The attenuation of radiation through a real atmosphere versus that through a clean dry atmosphere gives an indication of the atmospheric turbidity. Linke’s turbidity factor refers to the whole spectrum, i.e., overall spectrally integrated attenuation, which includes presence of gaseous, water vapor and aerosols, and indicates the number of ideal (clean and dry) atmospheres that produce the same extinction of the extraterrestrial solar beam as the real atmosphere. On the other hand the ngström turbidity coefficient is obtained from spectral measurements and is an indication only of the amount of aerosols in the atmosphere

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