4.8 Article

Importance of the description of light interception in crop growth models

期刊

PLANT PHYSIOLOGY
卷 186, 期 2, 页码 977-997

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OXFORD UNIV PRESS INC
DOI: 10.1093/plphys/kiab113

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资金

  1. Infrastructure Biologie Sante Phenome - National Research Agency [ANR-11INBS0012]
  2. EU Project Horizon 2020 Solutions for Improving Agroecosystem and Crop Efficiency [727247]
  3. H2020 Societal Challenges Programme [727247] Funding Source: H2020 Societal Challenges Programme

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This study analyzed the canopy light interception models of 26 wheat agricultural models and found that current models have not been evaluated with experimental data. Through field experiments, the K-ell(C) model was found to outperform current approaches under most lighting conditions, and the uncertainty in wheat growth and final yield due to light models could be as high as 45%. Therefore, there is a call for an overhaul of light interception models in crop growth models.
Canopy light interception determines the amount of energy captured by a crop, and is thus critical to modeling crop growth and yield, and may substantially contribute to the prediction uncertainty of crop growth models (CGMs). We thus analyzed the canopy light interception models of the 26 wheat (Triticum aestivum) CGMs used by the Agricultural Model Intercomparison and Improvement Project (AgMIP). Twenty-one CGMs assume that the light extinction coefficient (K) is constant, varying from 0.37 to 0.80 depending on the model. The other models take into account the illumination conditions and assume either that all green surfaces in the canopy have the same inclination angle (theta) or that theta distribution follows a spherical distribution. These assumptions have not yet been evaluated due to a lack of experimental data. Therefore, we conducted a field experiment with five cultivars with contrasting leaf stature sown at normal and double row spacing, and analyzed theta distribution in the canopies from three-dimensional canopy reconstructions. In all the canopies, theta distribution was well represented by an ellipsoidal distribution. We thus carried out an intercomparison between the light interception models of the AgMIP-Wheat CGMs ensemble and a physically based K model with ellipsoidal leaf angle distribution and canopy clumping (K-ell(C)). Results showed that the K-ell(C) model outperformed current approaches under most illumination conditions and that the uncertainty in simulated wheat growth and final grain yield due to light models could be as high as 45%. Therefore, our results call for an overhaul of light interception models in CGMs.

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