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Bragantia

Print version ISSN 0006-8705

Bragantia vol.71 no.4 Campinas  2012

http://dx.doi.org/10.1590/S0006-87052012000400016 

AGROMETEOROLOGY

 

Sensitivity of APSIM/ORYZA model due to estimation errors in solar radiation

 

Análise de sensibilidade do modelo APSIM/ORYZA na estimava de erros na radiação solar

 

 

Alexandre Bryan HeinemannI, *; Pepijn A.J. van OortII; Diogo Simões FernandesIII; Aline de Holanda Nunes MaiaIV

IEmbrapa Arroz e Feijão, Caixa Postal 179, 75375-000 Santo Antônio de Goiás (GO), Brasil
IIWageningen University, Department of Plant Sciences, Centre for Crop Systems Analysis, Wageningen, the Netherlands
IIISIMEHGO, Palácio Pedro L. Teixeira, Rua 82, s/nº, 2.º andar, Setor Sul, 74000-000 Goiânia (GO), Brasil
IVEmbrapa Meio Ambiente, Rodovia SP 340 - Km 127,5, 13820-000 Jaguariúna (SP), Brasil

 

 


ABSTRACT

Crop models are ideally suited to quantify existing climatic risks. However, they require historic climate data as input. While daily temperature and rainfall data are often available, the lack of observed solar radiation (Rs) data severely limits site-specific crop modelling. The objective of this study was to estimate Rs based on air temperature solar radiation models and to quantify the propagation of errors in simulated radiation on several APSIM/ORYZA crop model seasonal outputs, yield, biomass, leaf area (LAI) and total accumulated solar radiation (SRA) during the crop cycle. The accuracy of the 5 models for estimated daily solar radiation was similar, and it was not substantially different among sites. For water limited environments (no irrigation), crop model outputs yield, biomass and LAI was not sensitive for the uncertainties in radiation models studied here.

Key words: crop model, calibration, upland rice.


RESUMO

Modelos de simulação de culturas são importantes para quantificar riscos climáticos. Esses modelos necessitam de dados climáticos como dados de entrada. Entretanto, dados diários de precipitação pluvial e temperatura são facilmente encontrados, enquanto dados de radiação solar (Rs) limitam-se à aplicação de modelos de simulação de culturas. O objetivo deste estudo foi estimar a Rs utilizando cinco modelos de estimativa de radiação solar com base na temperatura do ar e quantificar a propagação de erros na radiação simulada na produtividade, biomassa, área foliar e radiação solar acumulada durante o ciclo da cultura do arroz de terras altas simulados pelo modelo de simulação ORYZA/APSIM. A acurácia dos cinco modelos de estimativa da radiação solar foi similar e não foi diferente entre os diferentes locais. Para ambientes que ocorre estresse hídrico, as saídas do modelo ORYZA/APSIM produtividade, biomassa e índice de área foliar não foram sensíveis às incertezas provenientes da radiação solar estimadas neste estudo.

Palavras-chave: modelos de simulação, calibração, arroz de terras altas.


 

 

1. INTRODUCTION

During the last decade, demand for rice in Brazil as well as in the world has increased considerably. However, the area available for rice production in the South of Brazil is limited, largely due to environmental and social constraints, such as competing demands for freshwater, industry or domestic use. Hence there is increasing interest in the upland rice systems of the Brazilian savannahs. This region is characterized by high inter and intra annual yield variability as consequence of precipitation patterns: even during the rainy season, there is chance of water stress occurrence due to periods of no rain or rain amount below crop demand. Thus, better quantification of existing climatic risks is urgently needed (MAIA et al., 2007) to provide the rice industry with information to better cope with existing climate variability and to adapt to likely future changes.

Crop models can be used to quantify effects of climate variability on yield variability and to explore options for coping with this variability (AKPONIKPÈA et al., 2011). The greatest limitation for crop model application in this region is the lack of climate data (HEINEMANN et al., 2008). Global radiation (Rs) is the driving factor controlling photosynthesis and evapotranspiration and is consequently an important weather variable for various agro-ecological studies. The lack of observed Rs data severely limits site-specific modelling of crop growth (DONATELLI et al., 2003). Rs at the earth surface depends on radiation at the top of the atmosphere (Ra) which can be calculated from latitude and day of year, based on astronomic equations. How much of Ra reaches the earth's surface depends on atmospheric transmissivity.

Several researchers have shown that atmospheric transmissivity can be estimated from maximum and minimum air temperatures (BRISTOW and CAMPBELL, 1984; DONATELLI and CAMPBELL, 1998; DONATELLI et al., 2003; HARGREAVES and SAMANI, 1985), with daily Rs estimated with accuracies of 50 to 98%, while FARHADI BANSOULEH et al. (2009) using the Hargreaves equations found strong interannual variation in accuracies, with R2 values ranging from 0 to 55%. As air temperature is recorded by all meteorological stations, temperature-based estimation methods are directly applicable in any region, provided that some years of Rs data are available for calibration of empirical parameters amongst these models, the Bristow-Campbell is the most commonly used. Much of this work on estimation of Rs is driven by the need for Rs as an input to crop growth models. Few studies however have quantified the impact of errors in Rs on errors in yields. Quite consistently, these studies conclude that yields can be accurately simulated, even with considerable error in Rs (FARHADI BANSOULEH et al., 2009; XIE et al., 2003). However, as the accuracy depends on the crop, environment and growth models used, results cannot be readly generalized for other scenarios.

The objective of this study are: i) to estimate solar radiation (Rs) in Goiás State, Brazil, by calibrating the models proposed by BRISTOW and CAMPBELL (1984), DONATELLI and BELLOCCHI (2001), DONATELLI and CAMPBELL (1998)(1), DONATELLI et al. (2003) and HARGREAVES and SAMANI (1985), and (ii) to quantify the propagation of errors in simulated Rs on several APSIM/ORYZA crop model seasonal outputs, namely: the upland rice yield, biomass, leaf area and total accumulated solar radiation during the crop cycle.

 

2. MATERIAL AND METHODS

APSIM/ORYZA Crop Model

ORYZA2000 is an explanatory, dynamic eco-physiological simulation model for rice (BOUMAN and VAN LAAR, 2006), integrated into APSIM (Agricultural Production Systems Simulator; KEATING et al., 2003). APSIM/ORYZA simulates rice phenology, leaf area development, biomass production, yield and nitrogen accumulation in response to environmental variables such as temperature, solar radiation, soil water content and nitrogen fertilizer management. In this study, water availability was simulated via APSIM-SoilWat2 module while crop water requirement, which is based on potential evapotranspiration, was computed in the APSIM-Eo module. The APSIM framework also includes a nitrogen and carbon dynamics module 'soilN'.

Solar Radiation Models

It was compared five models for estimating daily solar radiation (RS), namely: BC - BRISTOW and CAMPBELL (1984); HG - HARGREAVES (1981) modified by HUNT et al. (1998); CD(1); DB - DONATELLI and BELLOCCHI (2001) and modular model DCBB - DONATELLI et al. (2003). Four amongst these models (BC, CD, DB and DCBB) estimate the actual atmospheric transmissivity for the ith day of the year as a function of clear sky transmissivity (τ) and daily maximum (Tmax) and minimum (Tmin) temperatures. τ was assumed to be equal to 0.75 as suggested by FLETCHER and MOOT (2007).

where Ra is the daily potential radiation (MJ m-2 day-1), calculated with standard astronomic equations based on day of year and latitude (GOUDRIAAN and VAN LAAR, 1994) T = Tmax - (Tmin + Tmin+1)/2, T avg is the mobile week temperature based on centred mobile mean (as the average over 7 days around) of maximum and minimum temperature (ºC); and b and c are parameters separately calibrated for each site and model. In equations 2 - 4 two functions f1 and f2 are used:

where Tnc is the summer night temperature factor to avoid underestimation of solar radiation in summer (BECHINI et al., 2000); i= day of year, c1 and c2 are empirical model parameters for general seasonal factors (MAVROMATIS and JAGTAP, 2005). In the equation defining ƒ2(i), f3 is calculated as:

where c3 = c2 - integer(c2). Empirical parameters were calibrated using daily radiation data of the even years, for each of the stations listed in table 1. Next, the models were validated using the odd year data. The parameters b and c for BC, CD, DB and DCBB models were estimated by ordinary least squares. For HG model, they were fitted by nonlinear least squares via the iterative method based on Gauss-Newton algorithm by using MASS package from R software (R Development Core Team, 2012: http://www.r-project.org). Tnc, c1 and c2 parameters were fitted by ordinary least squares based on Tmin (Tnc) and day of year (c1 and c2) as described by BELLOCCHI et al. (2003) and DONATELLI et al. (2004). All parameters were calibrated for each weather station separately.

 

 

A number of researchers have shown that Rs values are also dependent on rainfall, altitude and latitude (HUNT et al., 1998, WEISS and HAYS, 2004). It was plotted radiation model residuals against rainfall to investigate whether the models were biased or more inaccurate at the high and low rainfall levels.

Data Collection and Crop Simulation

Daily maximum and minimum temperatures and global solar radiation data from weather stations in Goiás state (Table 1) were provided by the Meteorological and Hydrological System of Goiás State (SIMEHGO - "www.simego.sectec.go.gov.br/"). Data set available at each location ranged from 4 to 6 years. Data from even years was used for calibration of equations 1 to 8 and from odd ones for validation. The crop model APSIM/ORYZA for upland rice was calibrated to simulate crop responses environmental factors considering either observed or estimated solar radiation. Inputs to this model include daily weather data (minimum and maximum temperature, precipitation and solar irradiance), soil properties, initial soil water content, cultivar genetic characteristics, planting date, and N fertilizer management. The soil properties used as input for the crop model represent the most common soil type (Oxisols, covering 46% of the upland rice region, EMBRAPA, 1999). We used characteristics of the most commonly grown cultivar in the region, BRS Primavera (LORENÇONI et al., 2010). Model prognostic variables were simulated for nine locations and three planting dates, 1-Nov, 1-Dec and 31-Dec, corresponding to beginning, middle and end of planting season, respectively. The row spacing, plant density and nitrogen fertilization represent the local recommendation for upland rice in the region, 35 cm, 200 plant m-2 and 20 kg ha-1 of N at the planting date, 40 kg ha-1 at begin of tillering, and 40 kg ha-1 at begin of panicle initiation. Simulations started at least six months before each planting date in order to allow the establishment of a realistic soil water profile on the basis of rainfall patterns occurring before sowing because no irrigation was applied in the simulations. APSIM/ORYZA seasonal outputs analyzed in this study were yield; maximum accumulated biomass; maximum leaf area index (LAI) and accumulated solar radiation during the crop cycle (SRA).

Model validation

The accuracy of the solar radiation models was compared via descriptive statistics that indicate the degree of agreement between results based on either, monthly and daily observed or estimated solar irradiance as input data. The goodness of fit was assessed by the following measures: (i) parameter estimates (slope and intercept) of the regression line between estimated and measured values; (ii) correlation coefficient (r) (iii) the relative root mean squared error (RRMSE, equation 9), an indicator of the overall relative accuracy of the model; (iv) the systematic root mean square error (RMSEs), a measure of the model's linear (or systematic) bias (equation 10) and (v) the mean absolute error (MAE, equation 11), the arithmetic mean of absolute residuals. Small MAE values indicate a method with low overall mean error.

where Robs and Rest are, respectively, the observed and estimated daily solar radiation, n the number of days used for model fitting and is the best estimate of the predicted quantity calculated with the intercept (a) and slope (b) of the least-squares regression between Robs and Rest, = a + bxi.

To quantify the influence of inaccuracies in solar radiation estimates on APSIM/ORYZA seasonal outputs (Y) the model was run once a time using observed radiation or radiation estimated by each radiation model, resulting in a pair YR-obs and YR-est values for each radiation model and output variable. Differences between YR-obs and YR-est , here referred to as ΔY were then calculated for yield, biomass, maximum leaf area index (LAI) and accumulated solar radiation (SRA). We assessed the discrepancies between YR-obs and YR-est for each radiation model by several graphical and descriptive analysis: (i) box-and-whiskers plots of ΔY for displaying range of deviances, outliers and bias resulting from radiation estimation; (ii) deviance measures (r, MAE and RRMSE) previously described for evaluation of radiation models themselves and RMSE (root mean square error); (iii) similarity measures: the index of agreement d (WILMOTT, 1981; equation 12) and the coefficient of efficiency (NASH and SUTCLIFFE, 1970; equation 13) as joint measures of bias and accuracy and (iv) empirical cumulative distribution function (ecdf).

Thus what we present is a sensitivity analysis. The analysis shows how sensitive APSIM/ORYZA model output is to estimation errors in solar radiation. The accuracies reported therefore do not provide information on how good APSIM/ORYZA is at simulating actual yields. In this study model accuracy is considered excellent when RRMSE<10%; good if 10%<RRMSE<20%; fair if 20%<RRMSE<30%; and poor if RRMSE30% (JAMIESON et al., 1991); d and E are summary measures which accounts for accuracy. They range from 0 to 1 and minus infinity to 1, respectively. Basically, d represents the ratio between the mean square error and the "potential error" (WILLMOT, 1984) and E determines the relative magnitude of the residual variance ("noise") compared to the measured data variance ("information") (MORIASI et al., 2007). For both similarity measures, higher values indicate better agreement.

The ecdf functions for the observed (YR-obs) and estimated (YR-est) seasonal crop model outputs (yield, biomass, LAI and SRA) was calculated and the maximum vertical distance between YR-obs and YR-est ecdf's was determined by the Kolmogorov-Smirnov test (K-S).

 

3. RESULTS AND DISCUSSION

In the study region, the daily air temperature range increases from April, the beginning of the dry period, to August, which is the top of dry period and decrease from September, begin of the wet period, to December. For upland rice, the planting window is from November to December and rice is harvested in April. This period shows the lowest daily temperature range.

The local empirical parameter estimates obtained for the five models are described in table 2. Few papers actually report estimated values for these parameters. The parameter estimates listed here for the CD and DB models are similar to the ones described by BELLOCCHI et al. (2003). However, for the BC model, b parameter was higher (0.42 to 1.93) than the one reported in BELLOCCHI et al. (2003), ranging from 0.08 to 0.6. According to Liu et al. (2008), for the BC model, b parameter is more affected than c by different ways of calculating the monthly mean temperature (Tm) correction. In this study, Tm was calculated as centred week mobile average (Tavg ). Also we did not have set the c parameter as fixed for the BC model, but calibrated it separately for each location. Parameter c ranged from 1.12 to 1.89. For the HG model, parameters b and c are similar to those ones found by LIU et al. (2008). They ranged from 0.14 to 0.18 and -4.80 to 1.42, respectively.

The accuracy of the five models evaluated (Equations 1 - 5) was similar (Table 3): based on the average RRMSE values (Table 3) all were classified as good. The BC model showed the lowest mean RMSE and MAE values for calibration as well as validation. BC and CD model showed the lowest mean systematic error values (RMSEs) for calibration and validation. Considering all data set (Figure 1a - e), the r ranged from 0.72 to 0.75. These values are lower than the ones found in European studies (TRNKA et al., 2005), but similar to values presented in a Northern Australian study (LIU and SCOTT, 2000) and some values obtained from locations in North America (BALL et al., 2004). The CD model showed the highest degree of linear relationship between measured and simulated Rs (highest r value) followed by the BC and DB models (Figure 1b). Comparing the slopes and intercepts of the linear regressions between daily measured and predicted Rs, the HG model showed the slope (b) and intercepted (I) closest to 1 and 0, respectively, followed by the BC model (Figure 1a,e). The weekly aggregation of measured and predicted radiation values (Figure 1f - j) lead to increased r (0.81 to 0.86), minimizing the discrepancy. In this case, the BC and CD models showed the highest degree of agreement between measured and simulated Rs (highest r value) followed by the DB model. The BC model showed the slope and intercept closest to 1 and 0, respectively (Figure 1f). The highest residuals for all radiation models (Figure 1k - o)) corresponded to days with low rainfall values (<10 mm). The BC, CD, DB and DCDB models had the cubic smoothing spline regression parallel the zero residual line, showing no relationship between bias and rainfall. The HG and DCBB overestimated radiation under rainfall. Probably, adding rainfall variable in these two models will improve their performance under rainfall days.

Impact of estimated solar radiation on simulated crop model output

Considering pooled data from all weather stations, all evaluated radiation models (Equations 1 - 5) were classified in same class of accuracy (RRMSE<10%) for predicting yield, biomass and SRA (Table 4) which is not surprising considering that they simulated Rs with similar accuracies (Table 3). Only the HG model, for maximum LAI showed an RRMSE higher than 10%. In this study, all crop models outputs showed RMSE higher than MAE (Table 4). The ratio RMSE/MAE is an indicator of regression outliers (LEGATES and MCCABE, 1999). The highest difference between RMSE and MAE for yield was observed for BC model (80 kg ha-1) and the lowest for the HG model (68 kg ha-1). The HG model also showed the highest r for yield (0.99). All radiation models resulted in similar values for the index of agreement (d) for yield (Table 4). However, the coefficient of efficiency (E) for yield was different among models. Based on this index, the best models for estimated radiation to predict yield are BC, CD and DCBB. The use of daily solar radiation estimated by BC and HG as input to APSIM/ORYZA leads to overestimation of yield as characterized by boxes bellow the zero line (high frequency of YR-obs < YR-est) in Figure 2.

Conversely, when radiation was estimated via the CD, DB and DCBB models, the referred output variables showed an underestimation tendency. For maximum biomass, the highest difference between RMSE and MAE was observed for the DCBB model (151 kg ha-1) and the lowest for the BC model (92 kg ha-1). In this case the BC and HG models showed the highest r (0.97) (Table 4). Based on d, the best models were BC, CD and DCBB. Nevertheless, BC model showed the highest E. BC and HG models also leads to overestimate the maximum biomass as showed in Figure 2b, being the degree of overestimation higher for HG. For maximum LAI, the HG model accounted for the highest difference between RMSE and MAE (0.10) and the lowest difference by the BC and CD models (0.06). The BC and HG had the highest r values. According to d, the best models for maximum LAI were BC, CD and DCBB. Based on E, the best model was BC (Table 4). For this crop model output, BC and HG models showed the same trend as yield and biomass. Both models leads to overestimate the maximum LAI as showed in Figure 2c. However, the degree of overestimation is higher for the HG model. For SRA, the DCBB model accounted for the highest difference between RMSE and MAE (37 MJ m2 day-1). The CD model showed the lowest difference (20 MJ m2 day-1). The CD model also showed the highest r (0.65). According to d and E, the best model was BC (Table 4). For SRA, a quite different pattern was observed: radiation estimated via the BC, CD and DB models lead to simulated SRA values below the corresponding ones obtained by using observed radiation as model input. The HG and DCBB models showed an opposite tendency (Figure 2d). Taking into account the average of the deviance measures (RRMSE, RMSE, MAE and r) and similarity measures (d and E) for all crop models output studied here, the BC model had the lowest values for RRMSE, RMSE and MAE and the highest for r, d and E (Table 4).

The ecdf curve for YR-obs and YR-est seasonal crop model outputs were plotted in Figure 3. The quantile values derivate from ecdf for YR-obs and YR-est are showed in Table 5. For the seasonal crop model outputs yield, biomass and LAI, the ecdf curves for YR-obs and YR-est was quite similar (Figure 3a - c). It was also observed for the quantile values showed in table 5. Based on the K-S test, the ecdf curves for YR-obs and YR-est did not differ statistically at 10% of significance (Table 5, p value). It means that for a limited water environment (no irrigation) solar radiation is not the main driven for yield, biomass and LAI and soil water available has an important role for these crop model outputs. Then, crop model outputs yield, biomass and LAI are not sensitive for the solar radiation models studied here (BC, HG, DCBB and CD). Based also in the p value from K-S test (Table 5), the radiation model that showed the minimum vertical distance from YR-obs and YR-est ecdf curve for yield was BC and DCBB (p>0.05), for biomass and LAI was also BC model (p>0.05). For SRA, it was observed difference at level of 5% of significance between YR-obs and YR-est ecdf curve for DB, DCBB and HG solar radiation model (Table 5, p value). However, this difference in the accumulated solar radiation during the crop cycle was not enough to affected yield, biomass and LAI.

 

4. CONCLUSION

Five models for estimated daily solar radiation were tested in their agreement and showed similar accuracy (r=0.68 to 0.75, RMSE=12 to 14%). For water limited environments (no irrigation) the crop model outputs yield, biomass and LAI is not sensitive for the uncertainties in radiation models studied here (BC, CD, DB, HG and DCBB). Among the radiation models studied here, the BC model show the minimum vertical distance between YR-obs and YR-est ecdf's (highest p value) for all crop models outputs (yield, biomass, LAI and SRA).

 

ACKNOWLEDGEMENTS

To CNPq, for the support of the research project n. 471838/2008.

 

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Received: Aug. 21, 2012
Accepted: Dec. 5, 2012

 

 

* Corresponding author: alexandre.heinemann@embrapa.br
(1) As described in DONATELLI, M.; CAMPBELL, G.S. A simple model to estimate global solar radiation. In: CONGRESS OF THE EUROPEAN SOCIETY FOR AGRONOMY, 5., 1998, Nitra, Slovak Republic. Proceedings... [S.l.]: European Society for Agronomy, 1998. p.133-134.

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