International Journal of Applied Earth Observation and Geoinformation
Retrieval of wheat leaf area index from AWiFS multispectral data using canopy radiative transfer simulation
Introduction
Plant biophysical traits are generally used to model energy transfer processes between land and atmosphere (Bonan, 1991, Chen et al., 2007, Liu et al., 1997, Seller et al., 1997). Accurate crop leaf area index (LAI) is required as forcing parameter to predict the crop yield using crop simulation model and for efficient crop management at farm-scale. Any impact due to abiotic (e.g. temperature, water and nutrients) and biotic (e.g. pests and diseases) stresses would significantly change the crop LAI (Hameed et al., 2002, Jackson, 1986). Therefore, monitoring of LAI at farm to regional-scale is of practical importance for crop monitoring and agricultural management to settle damage claim under crop insurance. Satellite optical bands provide the spatial and temporal variation of spectral vegetation characteristics. The shape and form of canopy reflectance spectra depend on several factors like canopy structure, leaf biochemical composition, soil background and view and illumination geometry. The visible part of the canopy reflectance spectra is strongly controlled by leaf chlorophyll content (Gitelson et al., 2003). LAI has a large impact on reflectance spectra especially in the near-infrared (NIR) wavelength regions (Botha et al., 2007, Price and Bausch, 1995, Yi et al., 2008). Leaf water content is the primary determinant of canopy reflectance in the middle infrared (MIR) wavelength region.
Crop LAI can be estimated either from empirical models based on spectral vegetation indices (VIs) or through physically explicit canopy radiative transfer simulation model using inversion. Empirical models are generally restricted to site, time and crop. Therefore, these models cannot be extrapolated to large-scale for operational implementation (Baret and Guyot, 1991, Chaurasia et al., 2011, Colombo et al., 2003, Gobron et al., 1997). The physical models are proved as promising alternative because they describe the transfer and interaction of radiation within a canopy at regular spectral interval in optical region (Jacquemoud et al., 1996, Jacquemoud et al., 2000). These models provide an intrinsic connection between the plant biophysical characteristics and canopy reflectances. Various techniques have been proposed for the inversion of these models, including numerical optimization method (Jacquemoud et al., 1995, Jacquemoud et al., 2000), look-up table (LUT) approach (Combal et al., 2002) and neural network method (Danson et al., 2003, Leshno et al., 1993). The LUT approach is faster one and relies on a large set of database for the retrieval of specific variable. With the advancement in the efficiency of computational power, this methodology has the potential to retrieve the biophysical variables such as LAI, through inversion at various spatial scales.
Agriculture contributes approximately 14.2% in Gross Domestic Product (GDP) of India, whereas, wheat alone contributes 30.5% of total food production (Department of Agriculture and Cooperation, Ministry of Agriculture, Govt. of India, 2011). It is the dominant crop of north and north-central India during winter (rabi) season and the second highest staple food grain after rice. There is a wide variability in wheat grain productivity which varies between 1600 and 4600 kg ha−1 (Bhattacharya et al., 2011). Its yield prediction has a paramount importance in India to decide the import–export policies and minimum selling price for the farmers. The Ministry of agriculture, Government of India recently established a dedicated centre named Mahalanobis National Crop Forecasting Centre (MNCFC) (http://agricoop.nic.in) to provide crop acreage and production of major crops in advance on national scale. The operational pre-harvest yield forecast of crop such as wheat requires LAI as input to crop simulation model. The objectives of this study are (i) to develop a methodology for wheat LAI retrieval using CRT model and AWiFS (Advanced Wide Field Sensor) data, (ii) validation of retrieved LAI with in situ measurements and (iii) comparison of CRT retrieved LAI with empirical estimates from VI–LAI models.
Section snippets
Agro-climatic characteristics of study regions
The study area represents the two agro-climatic regions such as Trans-Gangetic Plain Region (TGPR) and Central Plain and Hills Region (CPHR). The TGPR is fully irrigated and the CPHR is partially irrigated. These regions represent the dominant wheat growing belts of north and central India including Punjab, Haryana and Madhya Pradesh provinces. Wheat is grown during middle of November of preceding year to late March (known as “rabi” season) in the following year with varying degree of
Pre-processing of satellite data and wheat map generation
Supervised hierarchical decision rule classifier was used to generate wheat distribution maps of two study regions (Oza et al., 2006a) using multi-date AWiFS data. The wheat area has been estimated using sample segment approach using radiometric normalization of data for clear day (Rajak et al., 2005) with RMSE of 0.5 pixel for geometric correction. This determination of wheat map generation has been evolved as a part of National Wheat Production Forecast (NWPF) project (Oza et al., 2006b).
The
Validation of MODIS atmospheric products
The MODIS eight-day atmospheric aerosol and water vapour were validated with in situ observations collected over a limited area during 2005–2006 and 2006–2007 wheat seasons. In situ diurnal AOD at 550 nm and water vapour were collected as per the sample design given for LAI in a 1000 m × 1000 m homogenous wheat patch. Average of 3 × 3 pixels were taken from resampled MODIS atmospheric product to validate with ground observations. The MODIS TERRA AOD at 550 nm showed root mean square deviation (RMSE) of
Discussion
All VIs with AWiFS spectral bands were able to capture the temporal gradient of LAI throughout the wheat season. The superiority of NDVI over other listed indices for the estimation of LAI produced no surprise as its mathematical formulation reduces maximum soil background and atmospheric perturbations as compared to others. But retrieval of LAI from simulation approach outperformed NDVI based LAI estimates at all LAI ranges and the most striking outcome was no ‘saturation’ of retrieved LAI for
Conclusions
The spatial resolution of AWiFS (56 m) is adequate enough to ensure relatively accurate retrievals of LAI of wheat crop at regional scale. The AWiFS has a 5-day revisit period which may cause loss of data due to persistent cloud or fog and to assess LAI at all major wheat growth stages. However, the combination of ResoureSat-1 and 2 increase the possibility to get clear sky data availability by reducing revisit period from 5 to approximately 2.5 days. The limitations of relatively low repetivity
Acknowledgments
The authors would like to thank Shri. A.S. Kiran Kumar, Director Space Applications Centre, ISRO for his encouragement, motivation and support throughout this study. The authors would also like to thank Dr. J.S. Parihar, Deputy Director, EPSA (SAC) for constant guidance. The authors also thank anonymous reviewers for their critical comments and wonderful suggestions that substantially improved the clarity of this paper.
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