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Winter Wheat Growth Spatial Variation Monitoring Through Hyperspectral Remote Sensing Image

机译:高光谱遥感影像监测冬小麦生长空间变化

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This work aims at quantifying the winter wheat growth spatial heterogeneity captured by hyperspectral airborne images. The field experiment was conducted in 2001 and 2002 and airborne hyperspectral remote-sensing data was acquired at noon on 11 April 2001 using an operational modular imaging spectrometer (OMIS). Totally 12 winter fields which covered by both dense and sparse winter wheat canopies were selected to analysis the winter wheat growth heterogeneity. The experimental semi-variograms for bands covered from invisible to mid-infrared were computed for each field then the theoretical models were be fitted with least squares algorithm for spherical model, exponential model. The optimization model was selected after evaluated by R-square. Three key terms in each model, the sill, the range, and nugget variance were then calculated from the models. The study results show that the sill, range and nugget for same field wheat were varied with the wavelength from blue to mid infrared bands. Although wheat growth in different fields showed different spatial heterogeneity, they all showed an obvious sill pattern. The minimum of mean range value was 7.52 m for mid-infrared bands while the maximum value was 91.71 m for visible bands. The minimum of mean sill value ranged from 1.46 for visible bands to 39.76 for NIR bands, the minimum of mean nugget value ranged from 0.06 for visible bands to5.45 for mid-infrared bands. This study indicate that remote sensing image is important for crop growth spatial heterogeneity study. But it is necessary to explore the effect of different wavelength of image data on crop growth semi-variogram estimation and find out which band data could be used to estimate crop semi-variogram reliably.
机译:这项工作旨在量化由高光谱机载图像捕获的冬小麦生长空间异质性。现场实验于2001年和2002年进行,并于2001年4月11日中午使用可操作的模块化成像光谱仪(OMIS)采集了机载高光谱遥感数据。选择了12个冬小麦田,覆盖了稀疏的冬小麦冠层,以分析冬小麦生长异质性。针对每个场计算了从不可见到中红外覆盖的波段的实验半变异函数,然后将理论模型与球面模型,指数模型的最小二乘算法进行拟合。通过R-square评估后,选择优化模型。然后,从模型中计算出每个模型中的三个关键项,门槛,范围和块金方差。研究结果表明,同一田间小麦的基石,幅度和矿块随波长从蓝色到中红外波段而变化。尽管不同田间小麦的生长表现出不同的空间异质性,但它们均表现出明显的基岩形态。中红外波段的最小平均值为7.52 m,而可见波段的最大值为91.71 m。平均基石值的最小值范围从可见波段的1.46到NIR波段的39.76,平均金块最小值的范围从可见波段的0.06到中红外波段的5.45。这项研究表明遥感图像对于作物生长空间异质性研究很重要。但是有必要探索图像数据的不同波长对作物生长半变异函数估计的影响,并找出哪些波段数据可以用来可靠地估计作物变异半函数。

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