Original papers
Solar radiation estimation methods using ANN and empirical models

https://doi.org/10.1016/j.compag.2019.03.022Get rights and content

Highlights

  • Hargreaves method to estimate solar radiation in two station of Greece.

  • Estimation of ANNs model to describe daily solar radiation.

  • Multi-linear regression models with different combination of input variables.

  • Comparison of Hargreaves, ANN and MLR models with data from two station.

Abstract

Many empirical equations and methods have been used and proposed in order to estimate the solar radiation (Rs). In this work, empirical equations, such as Hargreaves method, Artificial Neural Networks (ANN) technology and multi-linear regression methods (MLR) were used to estimate solar radiation. The daily meteorological measurements of air temperature, radiation, humidity and wind velocity from the stations of Aristotle University Farm and Amintaio in Northern Greece were used to derive the solar radiation models. The measurements of Rs were used to derive new and to evaluate existing models. Different combinations of input variables were examined in the ANN models, and in the MLR models different variables were used. The results of RMSE criteria of the examined models showed that they are in the same range with many other models describing Rs as summarized in many review articles. The use of extraterrestrial radiation and the square root of daily difference in temperature in the ANN and MLR models improve the accuracy of the results. The results of ANN models in comparison to MLR models using the same input variables are consistent between them.

Introduction

Solar radiation is critical in the design and operation of solar energy utilization systems, and it is one of the most significant parameters in reference evapotranspiration (ETo) estimation. The estimation of ETo is very interesting in agriculture, hydrology and ecology. The accuracy of solar radiation measurements and its respective estimations through models is then extremely important.

Numerous methods or equations have been developed and are being used to estimate the average monthly and daily solar radiation (Rs) in the last decades. These depend mainly upon the availability of meteorological data. For the designers and manufactures of solar equipment but also for other professionals, such as architects, agronomists and farmers, it is very important to have methods to indirectly estimate the solar radiation based on other readily available meteorological data (e.g. the actual and maximum sunshine duration, the average, maximum, minimum ambient temperature, the extraterrestrial radiation on horizontal surface (Ra), the longitude, altitude and latitude etc). The empirical methods of solar radiation and temperature based methods are considered as the most accurate methods to estimate ETo (Priestley and Taylor, 1972, Aschonitis et al., 2015, Antonopoulos and Antonopoulos, 2017).

The solar radiation is a meteorological variable which is not measured or is of low accuracy in many cases. Particularly in developing countries, solar radiation measurements are not easily available due to the cost, maintenance and calibration requirements of the respective equipment (Despotovic et al., 2015). In the Greek territory, many meteorological stations have been established in the last decade. Most of them do not measure solar radiation and thus the indirect estimation of solar radiation by other easily measured meteorological parameters is one alternative solution. Many models have been proposed and developed based on mathematical formulas, such as empirical models, artificial intelligence techniques (Zhang et al., 2017) and satellite-based methods. The empirical methods are divided into three groups (Zhang et al., 2017), the sunshine duration fraction models, the modified sunshine duration fraction models and the non-sunshine duration methods. The widely adopted Rs estimation models are based on sunshine duration and temperature datasets (Besharat et al., 2013). The most common Rs models are sunshine based (Allen et al., 1998), but the use of these models is often limited by the lack of available sunshine records. The temperature based models such as the Hargreaves model, are preferred in the absence of sunshine data.

The artificial intelligence techniques have being developed in recent decades to predict or forecast solar radiation. Artificial neural networks (ANN) have been used to accurately predict solar radiation by Yadav and Chandel, 2014, Kisi et al., 2015, Premalatha and Valan Arasu, 2016, Zhang et al., 2017 among many others. Zhang et al. (2017) reviewed and compared models, amongst of them the ANN models, from the points of view of time scale and estimation type.

Significant efforts for the accurate estimation of ETo under the Greek environmental-meteorological conditions have been carried out by several researchers. In many of them, the Rs estimation as the most significant input variable, has received special attention and was analyzed and examined (Alexandris et al., 2006, Valiantzas, 2006, Mavromatis, 2008, Ampas et al., 2007, Aschonitis et al., 2012, Paraskevas et al., 2013, Efthimiou et al., 2013, Valiantzas, 2018).

The aim of this study is to evaluate empirical equations as Hargreaves, Artificial Neural networks technology and multi-linear regression methods to estimate the solar radiation. The use of different input variables in the ANN and MLR models was evaluated based on measured Rs values. Daily data sets from two meteorological stations, in northern Greece were used.

Section snippets

Empirical methods

Hargreaves and Samani, 1982, Hargreaves and Samani, 1985 developed a simple model for estimating the incoming shortwave solar radiation Rs (MJ m−2 day−1), which requires only temperature data, as follows:Rs=KRS·Ra·TD0.5

where KRS is the adjustment coefficient of the radiation formula (°C−0.5), Ra is the extraterrestrial radiation (MJ m−2 day−1) and TD (equal to Tmax-Tmin) is the temperature difference between maximum (Tmax) and minimum (Tmin) daily temperature (°C). Hargreaves (1994) recommended

Results

The results of this work concern the use of the empirical equation of Hargreaves, the development of ANN models and the development of multiple-linear regression models for estimating solar radiation. Two sets of meteorological data from different regions in Northern Greece were used to develop and compare the models.

Discussion

The empirical equation of Hargreaves and models of Artificial Neural networks and multi-linear regression methods for estimating solar radiation were evaluated in this study based on the available datasets from two regions of Northern Greece. The results showed that these models have the ability to describe Rs with relatively high accuracy.

The comparison of the proposed ANN and MLR models showed that the MLR models performed better for the AUTH station, while the opposite was observed for the

Conclusions

The suitability of Hargreaves method, Artificial Neural networks (ANN) and multi-linear regression methods (MLR) to estimate solar radiation was evaluated using daily meteorological data from two stations in Northern Greece.

The results of these models were compared with measured Rs values. The results of RMSE criteria showed that they are in the same range with many other models describing Rs as summarized by Zang et al. in a review article of Rs models. The use of extraterrestrial radiation

Acknowledgements

The authors acknowledge Municipality of Amintaio and School of Agriculture of Aristotle University of Thessaloniki in Greece for providing the data sets of meteorological stations.

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