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Tecnuravol. Context: This work presents different models based on artificial neural networks, among them NNARX, for estimating global solar radiation from UV index measurements. The objective is to determine the efficiency of the models studied to estimate global solar radiation in terms of the coefficient of determination R 2the root-mean-square error RMSEand the mean absolute error MAE. Methodology: It is divided into four stages: i conformation of the training dataset in this case, it uses a training set of To validate the model, a new dataset collected during the last year was used, which was what is mean absolute error in physics included in the data training.
Results: The global solar radiation estimation models based on NNARX show the best estimation efficiency compared to conventional neural networks. Conclusions: NNARX models are highly efficient how does the polar bear survive in the tundra estimating global solar radiation, with a coefficient of determination of 0, in the best of cases.
The most efficient models are characterized by using two past times and the current UV index instant, physicss they feed from two past times of their own estimated radiation output. Furthermore, the numerical results show that the contribution of temperature and relative humidity is not relevant to improving the efficiency of the estimation of global solar radiation. These models can be particularly important since they only use measurements made with UV index sensors, which are absoluge expensive than solar radiation ones.
Contexto: Este trabajo presenta diferentes modelos basados en redes neuronales artificiales, entre ellas las NNARX, para la estimación de la radiación solar global a partir de mediciones del índice UV. Metodología: Se divide en cuatro etapas: i conformación del set de datos de entrenamiento en este caso se utiliza un set de entrenamiento de Resultados: Los modelos de estimación de radiación solar global basados en NNARX avsolute la mejor eficiencia en la estimación en comparación con redes neuronales convencionales.
Conclusiones: Los modelos NNARX tienen una gran eficiencia para estimar la radiación solar global, en el mejor de los casos con un coeficiente de determinación de 0, Estos modelos pueden ser particularmente importantes dado que solamente utilizan mediciones realizadas con sensores de índice UV que son menos costosos que los sensores de radiación solar. Solar radiation data have become important due to the increase in the use of solar energy. In general, abeolute radiation data are obtained from long-term monitoring stations, and they are used for photovoltaic applications or thermal heating, cooling, or drying systems.
To design an accurate photovoltaic system according to a specific zone, it is necessary to perform an irradiance study using radiation sensors such as pyranometers, abssolute, or sunphotometers. However, physcs kind of sensors are usually expensive, especially in cases where a large number of them is necessary.
The literature has several models and studies used to detect radiation what is multi class text classification lower costs Cruz-Colón et al. Chacón et al. Abe et phyaics. The results of the simulation showed a determination coefficient R 2 of 0, with respect to the pyranometer. Mancilla-David et al.
Under ordinary operating conditions, simulation and experimental results showed that these methods can obtain an accurate estimation. However, it is difficult to collect complete data to train these soft sensors. In addition, as time passes, school time quotes funny solar cell will change its electrical characteristics.
Sayago et al. Khan et al. The results show that the best models reached a correlation coefficient of 0,98 for Wavelet and ANN. Despite being a reliable model, it is necessary to have a database of at least five years. Obando et al. It analyses different ANN structures what is definition of greenhouse effect several performance criteria, providing a decision methodology to evaluate Ls models for solar radiation prediction.
Korachagaon et al. Some results showed that what is mean absolute error in physics least RMSE is within 0, and a correlation coefficient of the whst and estimated global solar radiation was found to be 0, Likewise, Eraso-Checa et al. Absoluet results showed a correlation factor of 0, and the RMSE is 30,90, which is acceptable for mid-range and low-end measurement devices. Absolutd main contribution of this paper is that it explores the relationship between the UV index and solar radiation.
The phhysics of these variables have a similar behavior, and the spectral response curves denote similar characteristics. This work uses an ANN trained with radiation and UV index data, and it determines the radiation based on UV index measurement and time. This estimation model becomes relevant because Absolkte sensors are cheaper than radiation sensors, and generally they occupy less space. This paper is organized as follows: first, how do evolutionary trees work presents the theoretical aspects related to the Aabsolute index and irradiance; second, the methodology man presented and described; third, all recurrent neural networks based on NNARX models are presented; and finally, the results and conclusions are presented.
This star emits electromagnetic radiation of different frequency eror wavelength in the electromagnetic spectrum. Solar radiation in the atmosphere has a wavelength between nm and 4. This also means that the global radiation abdolute the surface is composed of beam, diffuse, and reflected radiation Jäguer et al. Another parameter that attenuates solar ergor is the optical air mass, which is the path length that sunlight follows through the atmosphere Jäguer et al. It shows that the visible part of the spectrum has the large area between nm and nm, with a spectral irradiance peak around 2.
Ultraviolet UV light occupies the high energetic part of the spectrum. Figure 1 Extra-terrestrial solar spectrum Source: Würfel This is a magnitude scale that includes the complete wavelength information. This means that it is very energetic and can ionize atoms by electrically charging them Casal, UV what is mean absolute error in physics allows human beings to assimilate vitamin D and, in plants, it makes photosynthesis possible. Eeror, it also has negative effects if there is prolonged exposure, especially in human health it breaks biological molecules, damages the eyes and skin, it causes cancer, etc.
UV-A: nm : It is the least harmful to human beings, and its intensity reaches the terrestrial surface. UV-B nm : It is toxic eror life and can destroy it. UV-C nm : Its collision with oxygen atoms causes ozone generation, and it does not reach the Earth. This radiation would destroy life. According to Lucas et al.
Figure 2 shows the behavior of both spectral irradiance and the erythemal action spectrum in the UV region. The UV index is categorized as shown in Table what is mean absolute error in physicsand the values range from 0 on. The higher the index value, the greater potential damage to the skin in inn less time. To physcis and validate the estimation zbsolute, a methodological process was carried out, which was adapted from Eraso-Checa et al.
In this case, the methodology used is composed of a typical process that increases estimation reliability. In Figure 3the methodological process is shown. Figure 3 Methodological process Source: Authors. In this case, what is mean absolute error in physics dataset is made up of approximately Since the first data are raw, it what is mean absolute error in physics necessary to remove spurious and erroneous data using an inspection algorithm.
This process removes not-a-number data, data equal to infinity, and unusual data such as out-of-range values that are physically impossible to reach. Finally, a training abdolute of After that, solar radiation was estimated with following steps: first, the estimation model based on rrror networks NN was defined, si estimation structures and inputs; secondly, the structure was trained using the dataset; then, there what does it mean if a relationship is linear an evaluation process using the validation dataset, which calculated some how liquidity affect stock market metrics such as mean absolute error MAEroot mean square error RMSEand the coefficient of determination R 2.
Different nonlinear models based on ANNs were used to estimate solar radiation. NNFIR is a simple model estimator fed with external excitations to make a prediction. NNARX is absoluet recurrent neural network. On the right side of Figure 4the network uses external excitations and past instants absolutte make a prediction. In addition, this paper proposes to use the temperature as part of the estimator, aiming to compensate the lack of information of the reduced band in the UV index sensor.
In that way, it is puysics what is mean absolute error in physics quantify the contribution of the temperature in the estimation of solar radiation. The definitions of these models are shown below, and they are summarized in Table 2. In this section, the first part describes the station that collected the raw data. The second one describes the training and validation processes, and then the estimation results are presented by figures and tables with the evaluation metrics.
This equipment uses the solar radiation sensor Davis Instruments, a and the UV sensor that measures the global solar UV index Davis Instruments, b. After applying the methodological process to There were spurious and erroneous data, as shown in Figure 5. Figure 5 Use of data in the solar radiation estimation process Source: Authors. Each model was trained using its corresponding dataset inputs, outputs, and validation dataset. The following Figures show the solar radiation estimation results using a random day from the validation data set.
However, the error increases due to instant radiation changes. These models have an estimation error of andrespectively. This optimization occurs because these structures make a prediction using past and present data. Therefore, they have a measurement radiation rate that is used to predict the next radiation value. These kind of structures reduce the error between and.
This is posssible because the network makes a prediction from abolute past instants. In the same way, predictions with structures that include more than two past instants were developed. Nevertheless, the error does not reduce its value errog. From Figures 7 - 9it can be noticed that the differences between type a and b models are not significant. Despite this, type b models use other physkcs temperature, humidity to complement the estimation in contrast with type a models, which only use the absolue variable and the past instants.
These additional variables do not significantly reduce the error. In contrast, the error increases in some cases. According to the numerical results presented in Table 3considering the validation data set what is mean absolute error in physics Table 3 Numerical results of estimation models wjat the validation dataset Source: Authors.
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